Sternbild Sagittarius (Schütze)

Eigenschaften
Sagittarius ist ein helles und auffälliges Sternbild und liegt östlich von Scorpius und südlich von Aquila, in Richtung Zentrum unserer Galaxis, der Milchstraße, dessen fahl leuchtendes Band sich über den gesamten Himmel erstreckt. Die Fläche dieses Sternbilds beträgt 867 Quadtratgrad und das Zentrum kulminiert jeweils etwa am 5. Juli um Mitternacht. Manche erkennen in Sagittarius eine Milchkelle, welche die Milch der Milchstraße schöpft, doch das eindrücklichste Alignement in diesem Sternbild ist das des Teapot, einer Teekanne:
Im Spätsommer, wenn unter den kurzen, hellen Nächten endlich eine einmal wieder richtig dunkel klar ist, sieht man den Teapot im Süden mit aufgesetztem Deckel, dem Henkel im Osten und dem Ausguss im Westen. Im Laufe einer Nacht lässt sich verfolgen, wie der Teapot wie zum einschenken nach Westen verkippt und so scheint die helle, sternenreiche Region der Milchstraße wie zwei, drei Dampfwolken aus dem Ausguss aufzusteigen. Befindet man sich weiter südlich auf der Erdkugel, so ist auch der mit Milch aufgehellte Tee zu erahnen, der sich auf den Schwanz des Skorpions zu ergießen scheint. [9, 15]
Sterne mit Eigennamen:
- α Sgr: Rukbat, Rucba, Rukbat Al Rami, Alrami
- β1 Sgr: Arkab Prior, Arkab, Urkab
- β2 Sgr: Arkab Posterior, Arkab, Urkab
- γ2 Sgr: Nash, Alnasl, Alwazl, Zujj Al Nushshabah, Nushaba
- δ Sgr: Kaus Meridionalis, Kaus Media, Media
- ε Sgr: Kaus Australis
- ζ Sgr: Ascella
- λ Sgr: Kaus Borealis
- ν1 Sgr: Ain Al Rami
- π Sgr: Albaldah, Al Baldah
- σ Sgr: Nunki, Sadira
- ω Sgr: Terebellum
- 59 Sgr: Terebellum
IAU Name | Sagittarius |
IAU Genitiv | Sagittarii |
IAU Kürzel | Sgr |
Deutscher Name | Schütze |
Saison (47° N) | Mai … September |
Rektaszension | 17h 43m 12s … 20h 28m 41s |
Deklination | -45° 16' 39" … -11° 40' 34" |
Fläche | 867 deg2 |
Nachbarn (N↻) | Aql, Sct, Ser, Oph, Sco, CrA, Tel, Ind, Mic, Cap |
Deep-Sky Objektbeschreibungen
Messier 8
Messier 17
Messier 20
Messier 24
NGC 6445
Spinnennebel
NGC 6537
Galaxie
NGC 6822
Mythologie und Geschichte
Sagittarius ist ein altes Sternbild, das einen Zentauren mit Pfeil und Bogen darstellt. Zentauren sind Fabelwesen und sollen vor allem in Bergwäldern gelebt haben. Sie besitzen einen menschlichen Oberkörper auf dem Leib eines Pferdes.
In der griechischen Mythologie ist Ixion der Urvater der Zentauren. Der König der Lapithen in Thessalien, der einst - als geladener Tischgenosse bei den Göttern - der Hera, der Gattin des Zeus, in Lüsternheit Gewalt antun wollte. Doch Zeus ließ dies nicht zu und täuschte ihn mit einem Wolkengebilde, das aussah wie Hera. Dieser frevelhafte Versuch blieb allerdings nicht ungestraft und Ixion wurde in der Unterwelt auf ein sich ewig drehendes Rad gefesselt. Nephele ward Mutter und schenkte einem Wesen das Leben: dem Urzentaur. Ein wildes Geschöpf war dieser Pferdemensch, gewalttätig, weingierig, weibertoll und ungezügelt, voll von Trieben und nie befriedigt. Er schwängerte alle Stuten am Pelionberg in Thessalien und zeugte damit das Geschlecht der Zentauren. [20]

Eine besondere Ausnahme unter den Zentauren war Chiron, auch Crotus genannt. Er war der Sohn des Gauners Pan, welcher die Beine einer Ziege besaß, und Eupheme, die Amme der neun Musen. Chiron sang zur Leier als Dichter von der Entstehung der Erde und der Götter. Heilkräuter und Arzneien kannte er. Er war ein weises, hilfsbereites und gastfreundliches Wesen und war Erzieher vieler Helden und mancher Göttersöhne. Achilles, Asklepios und Herakles, sowie Orpheus und Jason, der Argonauten-Fahrer, waren darunter. Chiron gilt als der Erfinder des Bogens und der Pfeile und er war damit der erste Schütze. Chiron war unsterblich, denn Kronos hatte ihn einst in Pferdegestalt gezeugt. Doch als er einmal mit Heraklesan vergifteten Pfeilen hantierte, da drang versehentlich eine Pfeilspitze in Chirons Huf und verletzte ihn. Die Wunde bereitete ihm ständig unsagbare Schmerzen und er - der Unsterbliche - wünschte sich den Tod. Zeus versetzte ihn dann als Sternbild des Schützen an den Himmel. [20, 52, 80]
Nach [7] ist Sagittarius älteren Ursprungs als Centaurus und soll den grimmigen, ungezügelten Zentauren darstellen, der seinen Bogen auf Antares, dem Herz des Skorpion gerichtet hat, während Centaurus mit Chiron identifiziert wird.
Die Sumerer sahen in Sagittarius Negral, den Kriegsgott. Die Ägypter deuteten das Sternbild als Pfeil in einer menschlichen Hand. Vor 3000 Jahren sahen die Inder in dieser Sternkonfiguration ein Pferd, einen Pferdekopf und manchmal sogar einen Reiter. In vielen antiken Kulturen wurde die Milchstraße als jener Weg gesehen, den die Seelen nach dem Tod entlanggehen und Sagittarius repräsentierte den Torwächter des Todes. [20]
Kataloge
HR | B | F | DM | HD | SAO | FK5 | IR | M* | ADS | VarID | RA | Dec | vMag | spType | dMag | Sep ["] | Remarks |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
HR 6616 | 3 | CD-2711930 | 161592 | 185755 | 1464 | I | X Sgr | 17 47 33.6 | -27 49 51 | 4.54 | F7II | VAR:CDelta 4.24 - 4.84V, 7.01225d. | |||||
HR 6617 | BD-22 4423 | 161664 | 185765 | I | 9682 | 17 47 45.6 | -22 28 41 | 6.18 | G6IbHdel 1 | ||||||||
HR 6621 | CD-2612367 | 161756 | 185779 | V3894 Sgr | 17 48 27.8 | -26 58 30 | 6.35 | B4IVe | G:Sco-Cen assoc.,VAR:6.27 - 6.39V. Amp. 0.05V on time scale 3 hrs and 0.08 on time scale 1d suspected. | ||||||||
HR 6672 | CD-2413615 | 162978 | 185928 | 17 54 54.0 | -24 53 14 | 6.20 | O7.5II((f)) | G:Within 0.5d of HII reg. Ma 336.,S:Also classified O8III, O8IIIf, O8.5III((f)), O8II(f) O7.5II((f)) and O9.5Ib. uv 1394 and 1548 absorption very strong;,S:1548 emission weak. | |||||||||
HR 6679 | BD-18 4686 | 163245 | 160909 | 3423 | 17 55 55.0 | -18 48 08 | 6.52 | A4V | G:In cluster NGC 6494 #1. | ||||||||
HR 6680 | CD-2813878 | 163318 | 185975 | 17 56 41.9 | -28 03 55 | 5.80 | A7III/V: | ||||||||||
HR 6691 | CD-3612060 | 163652 | 209545 | W | 17 58 55.6 | -36 51 30 | 5.74 | G8III | 2.4 | 51.7 | D:Companion F0. | ||||||
HR 6692 | CD-2813936 | 163685 | 186025 | D | 17 58 39.1 | -28 45 33 | 6.01 | B3IV | 1.0 | 0.3 | D:Doubtful double, 6.3, 7.3v, sep. 0.3". | ||||||
HR 6693 | CD-3015035 | 163755 | 0 | I | W | A | 9929 | 17 59 05.2 | -30 15 11 | 5.16 | M1Ib | 1.8 | 5.5 | C:V magnitudes scatter from 4.98 to 5.14, B-V from +1.62 to +1.76, U-B from +1.52 to +1.93.,D:Fixed with HR 6694. Mag. and colors combined light, 4.98V, +1.63(B-V), +1.52(U-B).,VAR:4.96 - 5.00V for combined light with 6694. Uncertain which varies, probably 6693. | |||
HR 6694 | CD-3015035 | 163756 | 209553 | W | B | 9929 | 17 59 05.5 | -30 15 12 | 7.04 | G8II | 1.8 | 5.5 | D:Fixed with HR 6693. | ||||
HR 6700 | 4 | CD-2313731 | 163955 | 186061 | 3430 | 17 59 47.6 | -23 48 58 | 4.76 | B9V | ||||||||
HR 6704 | BD-20 4940 | 164028 | 186070 | D | 18 00 00.1 | -20 20 21 | 6.21 | K0II-III | D:Suspected occultation double. | ||||||||
HR 6708 | CD-3612115 | 164245 | 209608 | 18 01 48.3 | -36 22 40 | 6.30 | B7IV | ||||||||||
HR 6715 | 6 | BD-17 4987 | 164358 | 160998 | 1470 | I | 18 01 23.1 | -17 09 25 | 6.28 | K3III | |||||||
HR 6716 | BD-22 4503 | 164402 | 186135 | I | 10983 | 9996 | 18 01 54.4 | -22 46 50 | 5.77 | B0Ib | 7.1 | 8.2 | C:May not be the IR source. Strong IR excess probably due to circumstellar dust envelope. Color excess E(B-V) = +0.37.,G:Sgr OB1; in cluster M20.,S:Nitrogen deficient. | ||||
HR 6724 | 7 | CD-2413793 | 164584 | 186163 | 18 02 51.1 | -24 16 56 | 5.34 | F3III | G:NGC 6530 #4. | ||||||||
HR 6727 | BD-22 4516 | 164637 | 186169 | 18 03 01.7 | -22 43 06 | 6.74 | B0.5III | G:Sgr OB1. | |||||||||
HR 6736 | 9 | CD-2413814 | 164794 | 186204 | I | 18 03 52.4 | -24 21 38 | 5.97 | O4V((f)) | C:Color excess E(B-V) = +0.34.,G:Cluster NGC 6530 #7; Sgr OB1; in HII reg. S25; in nebulosity.,S:uv observations indicate dwarf; 1548 emission very strong. | |||||||
HR 6739 | CD-3512229 | 164870 | 209671 | 3435 | W | 18 04 50.4 | -35 54 05 | 6.00 | K2III | 5.2 | 12.5 | ||||||
HR 6742 | γ1 | CD-2914447 | 164975 | 186237 | 11029 | W Sgr | 18 05 01.3 | -29 34 48 | 4.69 | F4-G1Ib v | 0.0 | 0.1 | D:ADS 11029A is speckle interferometric double, sep. 0.116". Visual companions, 13.5v at 33" and 13.5v at 48".,N:Although HR 6742 and 6746 are named gamma1 and gamma2 Sgr, respectively, more often 6746 is simply called gamma Sgr,N:and the Greek letter is omitted for HR 6742.,SB:80y, K 2.65k/s, V0 -27.7k/s, asini 60.,VAR:ADS 11029A, CDelta 4.30 - 5.08V, 7.594710d. Period changes. Spectrum and magnetic field variable. One component of,VAR:SB. | ||||
HR 6746 | γ2 | 10 | CD-3015215 | 165135 | 209696 | 679 | I | 10173 | 18 05 48.5 | -30 25 27 | 2.99 | K0III | G:Wolf 630 group.,N:Nash; Alnasl; Alwazl; Zujj al Nushshabah; Nushaba. Gamma1 or gamma2 Sgr; see HR 6742. | ||||
HR 6748 | CD-3612214 | 165185 | 209710 | 18 06 23.7 | -36 01 11 | 5.95 | G5V | ||||||||||
HR 6762 | BD-21 4855 | 165516 | 186302 | 3438 | 18 07 11.4 | -21 26 38 | 6.28 | B0.5Ib | G:Sgr OB1; in HII region. | ||||||||
HR 6766 | CD-2814174 | 165634 | 186328 | 3439 | I | D | 18 08 05.0 | -28 27 26 | 4.57 | G7:IIIb* | 0.8 | 0.3 | D:5.1, 5.9, sep. 0.26", doubtful duplicity.,S:G7:IIIb CN-1 CH-3.5 HK1. Also classified G8IIIp CH-3 CN-2. Weak G-band. | ||||
HR 6769 | BD-17 5028 | 165687 | 161093 | I | 18 07 48.4 | -17 09 15 | 5.52 | K1III | |||||||||
HR 6772 | CD-3612265 | 165793 | 209779 | 18 09 22.4 | -36 40 21 | 6.58 | B1II | ||||||||||
HR 6773 | CD-2512793 | 165814 | 186350 | W | V3792 Sgr | 18 08 54.1 | -25 28 21 | 6.61 | B3III | 2.0 | 13.3 | D:Visual companion is blue.,SB:2.2481d, K 151k/s, V0 -6k/s, msin3i 6.42, asini 4.66. Mean mass components 5.5 solar.,VAR:EB 6.43 - 6.88V, 2.24815d. Mass transfer indicated. The var. is probably the 8.85V companion of the visual double. GCVS,VAR:gives combined light. | |||||
HR 6777 | CD-3213814 | 165978 | 209794 | 18 09 59.9 | -32 43 11 | 6.43 | K0IV | ||||||||||
HR 6780 | CD-3015316 | 166023 | 209803 | W | 18 10 05.7 | -30 43 43 | 5.53 | K1II | 2.3 | 3.9 | D:Binary. Combined mag., colors. Component B is F0IV or F0V.,RV:Comp. B, -17k/s.,S:Also classified K0IIIab. | ||||||
HR 6788 | CD-3312917 | 166197 | 209817 | 10304 | 18 10 55.2 | -33 47 59 | 6.16 | B1V | |||||||||
HR 6798 | BD-19 4886 | 166393 | 161153 | 11127 | 18 11 14.8 | -19 50 32 | 6.36 | A4V | 0.4 | 1.2 | D:AB visual double, A4V, F0, combined mag., color. Third component found by lunar occultation, 1.3B, 0.9R fainter than B,,D:sep. 0.024". | ||||||
HR 6801 | 11 | CD-2314047 | 166464 | 186437 | I | 11133 | 18 11 43.4 | -23 42 04 | 4.98 | K0III | 5.7 | 42.1 | D:Companion, 11.52V, +0.66(B-V), +0.11(U-B), F8V: | ||||
HR 6802 | CD-2814268 | 166469 | 186444 | V4045 Sgr | 18 11 58.2 | -28 54 05 | 6.51 | B9IVpSrEuCr | VAR:Amp. 0.013v, 2.8855d. | ||||||||
HR 6812 | μ | 13 | BD-21 4908 | 166937 | 186497 | 682 | 11169 | Mu Sgr | 18 13 45.8 | -21 03 32 | 3.86 | B8Iap e | 2.9 | 0.0 | D:ADS 11169A is SB, 4.1, 7.0v, sep. 0.011". Closest visual companion is B, 11.5v, B9III at 17"; C is 13.5v at 26";,D:D, 9.9v, B3; E, 9.4v, B2V, physical, vsini 184k/s.,G:Sgr OB1.,S:Shell star.,SB:ADS 11169A, 180.45d, K 56.8k/s, V0 -2.7k/s, asini 129.,VAR:ADS 11169A, EA 3.79 - 3.92V, 180.45d. Also irregular changes in brightness. | ||
HR 6816 | 14 | BD-21 4916 | 167036 | 186509 | I | 10393 | 18 14 15.9 | -21 42 47 | 5.44 | K3III | S:Case infrared spectra indicate M3. | ||||||
HR 6822 | 15 | BD-20 5054 | 167264 | 186543 | 18 15 12.9 | -20 43 42 | 5.38 | B0Ia | G:Sgr OB7; exciting star of HII region S35; NGC 6526. Also classified O9.7Iab. | ||||||||
HR 6823 | 16 | BD-20 5055 | 167263 | 186544 | 11191 | 18 15 12.9 | -20 23 17 | 5.95 | O9.5II v | 7.0 | 6.0 | D:Companion A3V.,G:Sgr OB7; exciting star of HII region S35; NGC 6526.,S:SiII suspected of variability. Also classified O9II, O9III and O9.5II-III((n)). | |||||
HR 6825 | BD-18 4864 | 167356 | 161227 | 11196 | 18 15 30.8 | -18 39 41 | 6.07 | A0Ia | 5.7 | 10.1 | D:Double may be spurious: companion not seen in 1934.,G:Sco-Cen assoc. | ||||||
HR 6832 | η | CD-3612423 | 167618 | 209957 | 683 | I | W | Eta Sgr | 18 17 37.6 | -36 45 42 | 3.11 | M3.5III e | 4.9 | 3.5 | S:Ultraviolet FeII emission.,VAR:Lb 3.08 - 3.12V. | ||
HR 6833 | CD-3412673 | 167647 | 209959 | W | RS Sgr | 18 17 36.1 | -34 06 26 | 6.16 | B3V+A | 2.6 | 94.1 | D:B, 9.68V at 39"; CD, 8.7, 10.2v, sep. 16.5".,S:Also classified B4IV.,SB:2.4157d, K 85.1k/s, V0 +6.0k/s, asini 2.82.,VAR:EA 6.0 - 6.9p, 2.4156832d. Period changes. Component A of visual double. | |||||
HR 6835 | CD-2814407 | 167666 | 186594 | 18 17 24.0 | -28 39 09 | 6.19 | A5/7V | ||||||||||
HR 6836 | CD-2814408 | 167665 | 186593 | 18 17 23.7 | -28 17 21 | 6.40 | G0V | ||||||||||
HR 6838 | BD-17 5112 | 167720 | 161260 | 3454 | I | 18 17 11.6 | -17 22 26 | 5.75 | K4II-III | ||||||||
HR 6841 | BD-18 4886 | 167771 | 161267 | W | 18 17 28.5 | -18 27 48 | 6.54 | O7III:(n)((f)) | 6.6 | 8.4 | D:Companion A3V, optical?,G:Sgr OB4; exciting star of HII region S41; within 0.5d of S39.,S:Also classified O7If and O8I(f).,SB:3.9735d, K1 107.1k/s, K2 122.9k/s, V0 +9.1k/s, m1sin3i 2.7, m2sin3i 2.3, a1sini 5.8,,SB:a2sini 6.7. | ||||||
HR 6842 | CD-2712684 | 167818 | 186612 | I | 18 18 03.2 | -27 02 33 | 4.65 | K3II | |||||||||
HR 6846 | CD-2512995 | 167979 | 186629 | I | 18 18 41.7 | -25 36 17 | 6.51 | gK1 | |||||||||
HR 6848 | BD-18 4896 | 168021 | 161304 | 11240 | 10543 | 18 18 43.3 | -18 37 10 | 6.84 | B0Ib | 0.5 | 0.4 | D:AB binary. C, 8.0v B0.5Ib at 18", vsini 42k/s.,G:Sgr OB4; exciting star of HII region S41; within 0.5d of S39. | |||||
HR 6859 | δ | 19 | CD-2914834 | 168454 | 186681 | 687 | I | 11264 | 18 20 59.7 | -29 49 41 | 2.70 | K3-IIIa* | 10.2 | 58.1 | N:Kaus Meridionalis; Kaus Media; Media.,S:K3-IIIa CN0.5 Ba0.2 Fe0.5. Also classified K3IIIa CN 1 Ba 0.1 Fe 0.5. | ||
HR 6861 | CD-2414219 | 168574 | 186699 | I | V4028 Sgr | 18 21 31.4 | -24 54 54 | 6.25 | M5III | R:Occult diam. = 0.0032". | |||||||
HR 6863 | BD-18 4926 | 168608 | 161376 | Y Sgr | 18 21 23.1 | -18 51 36 | 5.75 | F8I | RV:Possibly long period.,VAR:CDelta 5.40 - 6.10V, 5.77335d. | ||||||||
HR 6864 | CD-2814495 | 168646 | 186704 | 18 22 00.2 | -28 25 48 | 6.16 | A3III | S:Strong shell absorption; no emission. | |||||||||
HR 6870 | CD-3612524 | 168733 | 210061 | V4050 Sgr | 18 22 53.1 | -36 40 10 | 5.34 | Ap | G:Member of Pleiades group.,S:Chlorine in spectrum. Iron-rich star with overabundant titanium and chromium.,SB:11.7d. K =<0.5k/s.,VAR:Amp. 0.01v, 6.3d. Weak variable magnetic field, 14.6d. | ||||||||
HR 6874 | CD-3612537 | 168838 | 210075 | 18 23 28.9 | -36 14 18 | 5.55 | K0III | ||||||||||
HR 6879 | ε | 20 | CD-3412784 | 169022 | 210091 | 689 | W | 18 24 10.3 | -34 23 05 | 1.85 | B9.5III | 12.3 | 36.1 | N:KAUS AUSTRALIS.,R:Diam. = 0.00137 - 0.00144".,RV:Two discordant determinations of vsini, 0 and 175k/s. | |||
HR 6888 | 18 | CD-3015661 | 169233 | 210116 | I | 18 25 01.5 | -30 45 24 | 5.60 | K0III-IV | ||||||||
HR 6889 | CD-3612589 | 169236 | 210119 | 18 25 21.7 | -35 59 30 | 6.15 | K0III | ||||||||||
HR 6893 | CD-3412802 | 169398 | 210135 | 18 25 54.6 | -33 56 43 | 6.30 | B5IV | ||||||||||
HR 6896 | 21 | BD-20 5134 | 169420 | 186794 | I | 11325 | 18 25 21.0 | -20 32 30 | 4.81 | K2II | 3.6 | 1.7 | D:Companion is A5:.,DYN:0.006".,G:Red star Pleiades group. | ||||
HR 6907 | CD-2914965 | 169830 | 186838 | 18 27 49.5 | -29 48 59 | 5.92 | F9V | ||||||||||
HR 6909 | CD-2613184 | 169851 | 186837 | 11354 | 18 27 43.8 | -26 38 05 | 6.31 | A8V+F2V | 0.0 | 1.1 | D:Combined spectrum A5; component B, A8V:. | ||||||
HR 6913 | λ | 22 | CD-2513149 | 169916 | 186841 | 692 | I | 18 27 58.2 | -25 25 18 | 2.81 | K1+IIIb | G:Hyades group.,N:Kaus Borealis.,R:Occult diam. = 0.0044". | |||||
HR 6914 | CD-2613192 | 169938 | 186843 | 18 28 06.2 | -26 45 26 | 6.27 | A3/4V | ||||||||||
HR 6919 | BD-17 5203 | 169990 | 161493 | I | 10835 | 18 27 56.5 | -17 48 00 | 6.20 | B8V | ||||||||
HR 6926 | CD-2613206 | 170141 | 186863 | W | 10864 | 18 28 57.4 | -26 34 54 | 6.50 | A3III | 1.7 | 41.9 | VAR:Amp. 0.24V. | |||||
HR 6929 | CD-2513170 | 170235 | 186873 | V4031 Sgr | 18 29 22.0 | -25 15 23 | 6.59 | B2IVpe v | S:Shell star.,VAR:Amp. 0.10V. Spectrum (Balmer emission lines) variable. | ||||||||
HR 6933 | BD-18 4982 | 170433 | 161540 | 18 30 11.9 | -18 43 44 | 5.66 | gK0 | ||||||||||
HR 6936 | CD-3313281 | 170479 | 210257 | W | 18 31 04.8 | -32 59 21 | 5.34 | A3m | 4.5 | 3.4 | D:AB, CPM.,S:Also classified A3m. | ||||||
HR 6944 | BD-18 4988 | 170680 | 161564 | 11411 | 18 31 26.3 | -18 24 10 | 5.14 | A0Vp | 8.9 | 25.2 | D:Binary.,G:Hyades group.,S:Lambda Boo star, Ca, Mg 4481 wk. | ||||||
HR 6947 | BD-19 5047 | 170764 | 161571 | W | U Sgr | 18 31 53.3 | -19 07 30 | 6.68 | G1.5Ib | 2.0 | 430.7 | G:M25; in cluster IC 4725 #103.,VAR:CDelta 6.34 - 7.08V, 6.744925d. May have blue companion. | |||||
HR 6960 | CD-3313338 | 171034 | 210312 | 3471 | 18 33 57.8 | -33 01 00 | 5.28 | B2IV-V | G:Sco-Cen assoc. | ||||||||
HR 6961 | 24 | CD-2414472 | 171115 | 186981 | I | 18 33 53.5 | -24 01 57 | 5.49 | K4Ib | ||||||||
HR 6965 | 25 | CD-2414479 | 171237 | 186995 | 11035 | 18 34 32.8 | -24 13 21 | 6.51 | F3II-III | VAR:Delta Sct? | |||||||
HR 6969 | BD-20 5189 | 171369 | 187012 | 18 35 21.3 | -20 50 27 | 6.48 | F0IV | ||||||||||
HR 6972 | CD-2915123 | 171416 | 187024 | 3478 | 18 35 59.7 | -29 41 57 | 6.37 | K1III | |||||||||
HR 6988 | BD-21 5076 | 171856 | 187071 | 1485 | D | 18 37 54.4 | -21 23 52 | 5.94 | A8IIIn | 0.0 | 0.1 | D:Possible binary listed by D. W. Dunham, 6.5, 6.5, sep. 0.1". | |||||
HR 6990 | CD-2314572 | 171961 | 187080 | 18 38 30.7 | -23 30 18 | 5.81 | B8III | SB:Double lines suspected. | |||||||||
HR 6998 | BD-21 5081 | 172051 | 187086 | 18 38 53.4 | -21 03 07 | 5.86 | G4V | ||||||||||
HR 7011 | 26 | CD-2314625 | 172546 | 187146 | 3486 | 18 41 51.6 | -23 50 00 | 6.23 | Am | ||||||||
HR 7023 | BD-19 5134 | 172816 | 161754 | I | D | V3879 Sgr | 18 42 55.2 | -19 17 02 | 6.35 | M4III | 2.6 | 0.6 | D:Occultation double.,R:Occultation diam., two determinations, 0.0085" and 0.0101".,VAR:SRb 6.05 - 6.58p, about 50d. | ||||
HR 7026 | CD-3612946 | 172875 | 210507 | 18 44 07.7 | -36 43 07 | 6.32 | K0III | ||||||||||
HR 7029 | CD-3512876 | 172910 | 210509 | 3490 | W | 18 44 19.4 | -35 38 31 | 4.87 | B2.5V | 7.8 | 9.4 | G:Sco-Cen assoc.; member of the Sco-Cen cluster; member of Pleiades group. | |||||
HR 7035 | CD-2513394 | 173117 | 187216 | D | 18 44 49.6 | -25 00 40 | 5.83 | B5:V | 0.2 | 0.0 | D:Duplicity questionable.,G:Sco-Cen assoc.,SB:Suspected double, 6.4, 6.6v, sep. 0.04", probably SB. | ||||||
HR 7038 | BD-21 5131 | 173282 | 187234 | 18 45 18.7 | -21 00 05 | 6.36 | F5V | ||||||||||
HR 7039 | φ | 27 | CD-2713170 | 173300 | 187239 | 1487 | D | 18 45 39.4 | -26 59 27 | 3.17 | B8III | 0.0 | 0.1 | D:4.1, 4.1v, sep. 0.13", doubtful. | |||
HR 7045 | BD-19 5154 | 173425 | 161803 | I | 11309 | 18 46 01.2 | -19 36 23 | 6.42 | M4III | R:Diam. 0.0039".,VAR:Amp. 0.15V. | |||||||
HR 7046 | 28 | BD-22 4854 | 173460 | 187255 | I | 11652 | 18 46 20.6 | -22 23 32 | 5.37 | K4III | 7.7 | 13.7 | |||||
HR 7070 | CD-3413128 | 173902 | 210600 | 18 49 17.2 | -34 44 55 | 6.62 | K1IVCNIII | ||||||||||
HR 7072 | BD-18 5079 | 173928 | 161848 | W | 18 48 45.3 | -18 36 05 | 6.47 | G5III:+A0V: | 0.7 | 0.4 | |||||||
HR 7077 | BD-19 5182 | 174115 | 161871 | D | Var? | 18 49 35.5 | -19 08 32 | 6.75 | A1m | 0.0 | 0.2 | D:Suspected occultation double.,VAR:6.69 - 6.82V. | |||||
HR 7078 | 29 | BD-20 5277 | 174116 | 187324 | I | 11713 | 11372 | 18 49 40.1 | -20 19 29 | 5.24 | K4III | 8.6 | 16.6 | ||||
HR 7088 | 30 | BD-22 4881 | 174309 | 187342 | 1493 | 11731 | 18 50 50.5 | -22 09 44 | 6.61 | A7III | 6.8 | 21.1 | G:Hyades group. | ||||
HR 7103 | CD-2613562 | 174630 | 187388 | 18 52 28.5 | -26 39 01 | 6.29 | G8/K0III | ||||||||||
HR 7104 | CD-2915449 | 174631 | 187389 | 18 52 37.0 | -29 22 46 | 6.13 | K1III | ||||||||||
HR 7105 | CD-3016356 | 174632 | 210663 | 3502 | 18 52 41.7 | -30 44 03 | 6.63 | B8V | |||||||||
HR 7114 | 33 | BD-21 5176 | 174947 | 187422 | I | 18 54 00.1 | -21 21 35 | 5.69 | K1Ib | ||||||||
HR 7116 | ν1 | 32 | BD-22 4907 | 174974 | 187426 | I | 11794 | 18 54 10.2 | -22 44 42 | 4.83 | K2I+B9V: | 5.8 | 2.5 | D:AB fixed, combined mag., colors. C, 11.21V, +1.25(B-V), +1.20(U-B), at 28".,N:Ain al Rami. | |||
HR 7120 | ν2 | 35 | BD-22 4915 | 175190 | 187445 | I | 18 55 07.1 | -22 40 17 | 4.99 | K3II-IIIBa0.8CN2 | |||||||
HR 7121 | σ | 34 | CD-2613595 | 175191 | 187448 | 706 | I | W | 18 55 15.9 | -26 17 48 | 2.02 | B2.5V | 7.4 | 309.0 | C:Color excess E(B-V) = +0.02.,D:Interferometer measures indicate multiple star.,G:Sco-Cen assoc.,N:NUNKI; Sadira.,S:Lyman alpha and Lyman beta observed from COPERNICUS. | ||
HR 7126 | BD-16 5078 | 175317 | 161984 | 1495 | 18 55 31.0 | -16 22 36 | 5.79 | F4V | |||||||||
HR 7128 | CD-2314844 | 175360 | 187468 | 18 56 00.6 | -23 10 25 | 5.93 | B8 | ||||||||||
HR 7145 | ξ1 | 36 | BD-20 5339 | 175687 | 187498 | 18 57 20.5 | -20 39 23 | 5.08 | A0II | ||||||||
HR 7150 | ξ2 | 37 | BD-21 5201 | 175775 | 187504 | 710 | I | 18 57 43.8 | -21 06 24 | 3.51 | K1III | R:Occultation diam. = 0.0030 - 0.0042". | |||||
HR 7151 | CD-3116189 | 175794 | 210773 | 18 58 21.3 | -31 02 10 | 6.12 | K3III | ||||||||||
HR 7155 | CD-2513574 | 175852 | 187517 | D | 18 58 20.5 | -24 52 36 | 6.62 | A0 | 0.0 | 0.1 | D:Suspected occultation double, equal components. | ||||||
HR 7159 | BD-22 4928 | 175892 | 187519 | 18 58 24.6 | -22 31 46 | 6.14 | A2V | ||||||||||
HR 7164 | BD-18 5155 | 176123 | 162050 | D | 18 59 26.8 | -18 34 01 | 6.37 | G3II | D:Suspected occultation double. | ||||||||
HR 7166 | BD-13 5172 | 176162 | 162052 | W | Var | 18 59 23.8 | -12 50 26 | 5.53 | B5IV | 0.5 | 0.4 | D:Binary. B1, B9.,VAR:Amp. 0.053B. | |||||
HR 7168 | CD-2513614 | 176246 | 187562 | 19 00 24.8 | -24 56 32 | 6.36 | gK0 | ||||||||||
HR 7182 | BD-22 4946 | 176537 | 187584 | I | 19 01 37.8 | -22 41 44 | 6.24 | K5 | |||||||||
HR 7186 | BD-15 5185 | 176593 | 162097 | 19 01 33.5 | -15 16 57 | 6.32 | gG6 | ||||||||||
HR 7194 | ζ | 38 | CD-3016575 | 176687 | 187600 | I | 11950 | 19 02 36.7 | -29 52 49 | 2.60 | A2III+A4IV | 0.3 | 0.5 | D:AB 3.2 A2III, 3.4 A2V, 21.138y, a = 0.532".,DYN:0.040".,N:Ascella. | |||
HR 7195 | CD-2513655 | 176704 | 187599 | D | 19 02 27.7 | -24 50 49 | 5.65 | K3III | 0.0 | 0.1 | D:Suspected occultation double with equal components; combined mag., color.,G:Arcturus group.,R:Occultation diam. under 0.002". | ||||||
HR 7203 | BD-19 5273 | 176884 | 162130 | 11972 | 19 03 03.8 | -19 14 43 | 6.05 | G6III | 3.5 | 7.4 | D:AB CPM. B, 9.17V, +0.47(B-V), +0.09(U-B). | ||||||
HR 7205 | BD-19 5275 | 176903 | 162133 | D | 19 03 07.0 | -19 06 12 | 6.37 | F5IV-V | 0.0 | 0.1 | D:Probable double, 7.1, 7.1v, sep. 0.05". | ||||||
HR 7211 | CD-3116306 | 177074 | 210883 | 19 04 25.1 | -31 02 49 | 5.50 | A0IV | ||||||||||
HR 7217 | ο | 39 | BD-21 5237 | 177241 | 187643 | I | 11996 | 11703 | 19 04 41.0 | -21 44 30 | 3.77 | G9IIIb | 9.9 | 35.7 | |||
HR 7230 | BD-15 5223 | 177517 | 162177 | 3522 | W | Var? | 19 05 41.2 | -15 39 37 | 5.97 | B9V | 6.2 | 46.9 | S:Sp. shows Hg, Si.,VAR:Variable on short time scale with uncertain 0.33772d period. Manfroid and Mathys (1985, A&AS, 59, 429) also give,VAR:possible 0.48773d period. Magnetic field not detected (Borra and Landstreet 1980, ApJS, 42, 421). | ||||
HR 7234 | τ | 40 | CD-2713564 | 177716 | 187683 | 1496 | I | 19 06 56.4 | -27 40 14 | 3.32 | K1+IIIb | G:Possibly Wolf 630 group. | |||||
HR 7239 | BD-16 5153 | 177817 | 162201 | 12039 | 19 06 52.3 | -16 13 44 | 6.03 | B8IV | 4.0 | 6.4 | D:Companion A0V. | ||||||
HR 7240 | CD-2815403 | 177846 | 187701 | I | 19 07 30.9 | -28 38 13 | 6.04 | K3III | |||||||||
HR 7241 | BD-18 5206 | 177863 | 162204 | 11743 | 19 07 08.5 | -18 44 16 | 6.29 | B8III | |||||||||
HR 7246 | CD-2415041 | 178075 | 187718 | 19 08 14.6 | -24 39 25 | 6.30 | B9III | ||||||||||
HR 7249 | BD-19 5312 | 178175 | 162229 | V4024 Sgr | 19 08 16.7 | -19 17 24 | 5.54 | B2Ve v | S:H alpha variable.,VAR:Amp. 0.2V. | ||||||||
HR 7256 | CD-3613355 | 178299 | 210996 | 3528 | 19 09 36.4 | -36 09 53 | 6.56 | A0IV | SB:Nearly equal components. Period probably long. | ||||||||
HR 7264 | π | 41 | BD-21 5275 | 178524 | 187756 | 720 | I | W | 11769 | 19 09 45.8 | -21 01 25 | 2.89 | F2II | 0.0 | 0.1 | D:AB, combined mag., colors, sep. 0.093". Third component 6.0v at 0.4".,G:Red star Pleiades group.,N:Albaldah; Al Baldah. | |
HR 7265 | BD-20 5415 | 178555 | 162260 | 12096 | 19 09 48.1 | -19 48 13 | 6.13 | K1III | 0.2 | 0.1 | D:7.0 K3III, 7.2 K2III. Unresolved by speckle interferometry. Probably not double. | ||||||
HR 7270 | CD-2915804 | 178840 | 187786 | 19 11 18.9 | -29 30 08 | 6.30 | B9 | ||||||||||
HR 7276 | BD-21 5292 | 179201 | 187816 | 19 12 28.0 | -21 39 29 | 6.41 | gG8 | ||||||||||
HR 7277 | CD-2613936 | 179323 | 187835 | 3533 | I | 19 13 13.7 | -25 54 24 | 5.80 | K1I | ||||||||
HR 7282 | BD-12 5311 | 179497 | 162326 | 3534 | I | 11815 | 19 13 15.5 | -12 16 57 | 5.51 | gK4 | |||||||
HR 7291 | CD-2415161 | 179949 | 187883 | 19 15 33.2 | -24 10 45 | 6.25 | F9V | ||||||||||
HR 7292 | ψ | 42 | CD-2513866 | 179950 | 187882 | I | 12214 | 19 15 32.4 | -25 15 24 | 4.85 | G8:III+A8V | 0.3 | 0.1 | C:Probably not IR source.,D:5.5 F8V, 5.7 F9V, 18.75y, a = 0.153". Component A is SB, 6.2, 6.2v, sep. 0.001".,DYN:0.010".,S:AB variously classified as F2:+F7III, F8V+F9V, F6V+F7V, A8V+G8:III.,SB:ADS 12214B, SB2O 10.7786d, K 72.5k/s, V0 -43.0k/s, asini 9.48. Masses 2.1 and 1.7 solar. ADS 12214AB, 7319.0d, K,SB:10.0k/s, V0 -26.8k/s, msin3i 3.78, asini 866. A, 2.7 solar mass. | |||
HR 7296 | CD-3314076 | 180093 | 211117 | I | RY Sgr | 19 16 32.8 | -33 31 18 | 6.25 | G0Ipe(C1,0) | C:Possible extinction by circumstellar dust.,M:Possibly high luminosity evolved helium star.,RV:38.6d.,S:Hydrogen deficient carbon star.,VAR:RCB 6.0 - >15.0v. Also pulsations 38.454d, changing amplitude. Observations 1984-86 indicate semiregular pulsations,VAR:of 33 to 40d, 6.13 - 6.78V, 0.38 - 0.76(B-V), -0.09 to +0.52(U-B). | |||||||
HR 7304 | 43 | BD-19 5379 | 180540 | 162413 | 722 | D | 19 17 38.1 | -18 57 11 | 4.96 | G8II-III | D:Suspected occultation double.,R:Diam. 0.0018". | ||||||
HR 7316 | CD-3513393 | 180885 | 211175 | 1501 | 19 19 40.0 | -35 25 17 | 5.59 | B3V | G:Sco-Cen assoc.; Sco-Cen cluster? | ||||||||
HR 7317 | BD-15 5310 | 180928 | 162462 | I | W | 19 19 00.1 | -15 32 11 | 6.06 | K3III | 5.5 | 48.6 | ||||||
HR 7323 | CD-3215071 | 181109 | 211191 | I | 19 20 26.2 | -31 49 04 | 6.58 | M0III | |||||||||
HR 7327 | BD-22 5063 | 181240 | 187992 | 19 20 38.1 | -22 24 09 | 5.58 | F0III: | ||||||||||
HR 7330 | CD-3513422 | 181321 | 211206 | 19 21 29.9 | -34 59 02 | 6.48 | G5V | VAR:Nearby star suspected of variability from photometric discordances by different observers. | |||||||||
HR 7334 | CD-4214133 | 181401 | 229643 | 19 22 09.6 | -42 00 58 | 6.34 | K1III | ||||||||||
HR 7337 | β1 | CD-4413277 | 181454 | 229646 | 1502 | W | 19 22 38.3 | -44 27 32 | 4.01 | B9V | 3.3 | 28.3 | D:CPM. Companion A5V; vsini 129k/s, optical?,N:Arkab Prior; Arkab or Urkab with HR 7343. | ||||
HR 7339 | BD-19 5412 | 181558 | 162511 | W | 19 21 37.1 | -19 14 03 | 6.26 | B5V | 3.6 | 90.8 | D:Component B, K2IV, RV -3; component C, G5:III, optical. | ||||||
HR 7340 | ρ1 | 44 | BD-18 5322 | 181577 | 162512 | D | Rho1 Sgr | 19 21 40.4 | -17 50 50 | 3.93 | F0IV-V | 2.5 | 0.0 | D:Sep. 0.036". Questionable occultation double.,G:Possible Eggen group with HR 63, q.v.,VAR:Delta Sct 3.90 - 3.93V, 0.050d. | |||
HR 7342 | υ | 46 | BD-16 5283 | 181615 | 162518 | 727 | I | D | Ups Sgr | 19 21 43.6 | -15 57 18 | 4.61 | B2Vpe+A2IaShell v | 1.0 | 0.0 | C:Large IR excess.,S:Hydrogen deficient, strong carbon? Also classified B8+F2p, B8I, F0Ia, and Apep + O9V. H alpha variable.,SB:4.8, 5.8v, sep. 0.011", 137.9567d, K 49.1k/s, V0 +13.3k/s, asini 93.0. Analysis of IUE data by Dudley and,SB:Jeffery (1990, MNRAS, 247, 400) gives a K2 velocity of 29.7k/s and a mass ratio of 0.63+/-0.01, indicating that,SB:upsilon Sgr is a strong candidate as a progenitor of a type Ib supernova.,VAR:EB 4.34 - 4.44p, 137.939d. Irregularities in light variation. Variable polarization, probably due to circumstellar,VAR:dust. | |
HR 7343 | β2 | CD-4513171 | 181623 | 229654 | 19 23 13.2 | -44 47 59 | 4.29 | F2III | N:Arkab Posterior; Arkab or Urkab with HR 7337. | ||||||||
HR 7344 | ρ2 | 45 | BD-18 5325 | 181645 | 162521 | 19 21 50.9 | -18 18 30 | 5.87 | gG9 | ||||||||
HR 7348 | α | CD-4013245 | 181869 | 229659 | 728 | 19 23 53.2 | -40 36 58 | 3.97 | B8V | N:Rukbat; Rucba; Rukbat al Rami; Alrami. | |||||||
HR 7350 | CD-4313352 | 181925 | 229660 | 19 24 21.4 | -43 43 23 | 6.17 | M1-2III | ||||||||||
HR 7355 | CD-2815767 | 182180 | 188079 | 19 24 30.1 | -27 51 56 | 6.04 | B2Vn | G:Sco-Cen assoc. | |||||||||
HR 7360 | CD-2916104 | 182286 | 188093 | 12400 | 19 25 04.1 | -29 18 33 | 5.93 | K3III | 4.4 | 12.1 | D:Optical. | ||||||
HR 7362 | χ1 | 47 | CD-2415303 | 182369 | 188101 | W | 19 25 16.5 | -24 30 31 | 5.03 | Am | 0.0 | 0.1 | D:5.8 A8, 5.8 A6-F0, 10.8y, a = 0.123". Probable occultation double. Speckle interferometry 1985.5 gives sep. 0.081".,N:Chi1 Fl 47, Chi2 Fl 48 and Chi3 Fl 49 Sgr are, respectively, HR 7362, HD 182391 (7.08v, B9) and HR 7363.,G:Hyades group.,S:K/H/met give A5/F0V/F0. | ||||
HR 7363 | χ3 | 49 | CD-2415307 | 182416 | 188105 | I | 11992 | 19 25 29.7 | -23 57 44 | 5.43 | K4III | ||||||
HR 7367 | BD-14 5428 | 182477 | 162595 | 3552 | I | 19 25 21.6 | -13 53 49 | 5.69 | K3III | ||||||||
HR 7375 | 50 | BD-22 5105 | 182629 | 188121 | 3553 | I | 19 26 19.2 | -21 46 36 | 5.59 | K3III | |||||||
HR 7378 | BD-15 5348 | 182645 | 162609 | 19 26 11.1 | -15 03 11 | 5.72 | B8Vn t | VAR:H alpha emission variable. | |||||||||
HR 7379 | BD-14 5435 | 182678 | 162615 | 19 26 24.6 | -14 33 04 | 6.70 | A1V | ||||||||||
HR 7380 | CD-2916140 | 182681 | 188127 | 731 | 19 26 56.5 | -29 44 36 | 5.67 | B9V | |||||||||
HR 7392 | CD-4313395 | 183007 | 229712 | 19 29 23.9 | -43 26 45 | 5.71 | Am | S:Also classified A3p.,SB:164.64d, K 11.8k/s, V0 -30.9k/s, asini 26.5. | |||||||||
HR 7398 | CD-2714004 | 183275 | 188192 | I | 12506 | 19 29 52.2 | -26 59 08 | 5.52 | K3III | 3.5 | 7.6 | D:Binary. B, 8.69V, +0.86(B-V), +0.32(U-B), G1IV-V.,DYN:0.011".,G:Hyades group.,S:Also classified K2IIIab. | |||||
HR 7399 | CD-3215233 | 183312 | 211315 | 19 30 14.7 | -32 05 32 | 6.60 | F3IV-V | ||||||||||
HR 7410 | BD-21 5410 | 183545 | 188219 | 19 30 54.0 | -21 18 44 | 6.13 | A2 | ||||||||||
HR 7422 | CD-4013356 | 184035 | 229746 | 3560 | V4089 Sgr | 19 34 08.5 | -40 02 05 | 5.89 | A3III | SB:4.625d, K 72.5k/s, V0 +11.9k/s, asini 4.59. Masses 3 and 2 solar. Primary overluminous for its mass; secondary may,SB:be neutron star.,VAR:E, amp. 0.13V, 4.62988d. | |||||||
HR 7431 | 51 | CD-2415442 | 184552 | 188326 | 12183 | 19 36 01.7 | -24 43 09 | 5.65 | A7m | 2.0 | 0.0 | SB:5.9, 7.9v, sep. 0.0002", 8.1158d, K 20.9k/s, V0 -30.3k/s, asini 2.31.,VAR:Primary of SB Delta Sct? Amp. 0.015V in about 10d. | |||||
HR 7433 | BD-12 5461 | 184574 | 162797 | 19 35 33.6 | -12 15 10 | 6.27 | K0 | ||||||||||
HR 7439 | BD-19 5521 | 184705 | 162809 | 19 36 26.1 | -18 51 10 | 6.11 | F0III | ||||||||||
HR 7440 | 52 | CD-2514184 | 184707 | 188337 | 736 | 12654 | 12191 | 19 36 42.4 | -24 53 01 | 4.60 | B9 | 4.5 | 2.7 | D:CPM.,VAR:ADS 12654. Uncertain which component varies. | |||
HR 7443 | BD-18 5432 | 184835 | 162816 | 3565 | 19 37 03.3 | -18 13 52 | 5.64 | K3III | |||||||||
HR 7454 | BD-14 5479 | 184985 | 162827 | 19 37 34.4 | -14 18 06 | 5.47 | F5V | SB:Unresolved by speckle interferometry 1986.46. | |||||||||
HR 7464 | CD-3913371 | 185257 | 211451 | V4090 Sgr | 19 39 55.7 | -39 26 00 | 6.61 | A2m | S:Also classified A7V. | ||||||||
HR 7470 | 53 | CD-2315618 | 185404 | 188407 | 12741 | 19 39 49.4 | -23 25 40 | 6.34 | B9.5V+A3IV | 0.2 | 0.2 | D:Sep. 0.200". | |||||
HR 7473 | CD-2315625 | 185467 | 188419 | 19 40 07.1 | -23 25 43 | 5.97 | gK1 | ||||||||||
HR 7476 | 54 | BD-16 5399 | 185644 | 162883 | 1512 | I | 12767 A | 12275 | 19 40 43.4 | -16 17 36 | 6.20 | K2III+F8V | 0.0 | 0.1 | D:Primary is close double, combined colors. Mag. for blend 5.30V. Component B, 12.6v at 38" optical. C, 8.9 F8V,D:at 46" physical.,VAR:Amp. 0.09V. | ||
HR 7489 | 55 | BD-16 5413 | 186005 | 162915 | 1514 | W | 19 42 31.1 | -16 07 26 | 5.06 | F1III | 0.0 | 0.2 | D:Suspected visual double, but may be single. | ||||
HR 7491 | CD-3713322 | 186042 | 211506 | 3576 | 19 43 37.6 | -37 32 20 | 6.16 | B8 | |||||||||
HR 7496 | BD-15 5444 | 186185 | 162931 | W | 19 43 33.5 | -15 28 12 | 5.49 | F5IV | 6.2 | 70.4 | RV:Over 1500d. | ||||||
HR 7507 | CD-3215443 | 186500 | 211541 | 1516 | 19 46 01.2 | -31 54 31 | 5.52 | B8V | |||||||||
HR 7515 | 56 | BD-20 5698 | 186648 | 162964 | 1517 | I | 19 46 21.7 | -19 45 40 | 4.86 | K1III | |||||||
HR 7532 | BD-14 5555 | 186984 | 162998 | 19 48 03.0 | -13 42 12 | 6.11 | A6m | ||||||||||
HR 7538 | CD-2916546 | 187098 | 188603 | 3582 | 12956 | 19 49 11.6 | -28 47 20 | 6.05 | F2V | D:6.1, 11.9v sep. 2" in 1910, 1913, not seen as double in 1926, 1928, 1929. Probably single? | |||||||
HR 7552 | CD-4013514 | 187474 | 229903 | 3583 | V3961 Sgr | 19 51 50.6 | -39 52 28 | 5.33 | A0pCrSr: v | SB:690d.,VAR:5.28 - 5.33V, 2445.2d. Revised period 2300d. Variable magnetic field and spectrum. | |||||||
HR 7561 | 57 | BD-19 5631 | 187739 | 163060 | 19 52 12.0 | -19 02 42 | 5.92 | G5III | |||||||||
HR 7571 | BD-14 5578 | 187949 | 163080 | S | V505 Sgr | 19 53 06.4 | -14 36 11 | 6.48 | A0V+F8IV | 0.3 | D:Speckle interferometry indicates companion at 0.291", probably not the same as the SB or occultation binary.,SB:6.6 - 8.6v, sep. 0.0002", 1.1829d, K 104k/s, V0 -2k/s, asini 1.69; vsini of secondary 50k/s.,VAR:EA 6.48 - 7.51V, 1.18287511d. Period decreases about 0.49s/y. i 80.3d. Contact binary. Masses 2.2 and 1.2 solar, radii,VAR:both about 2.2. | ||||||
HR 7578 | CD-2415668 | 188088 | 188692 | 13072 | Var? | 19 54 17.7 | -23 56 28 | 6.18 | K2V | 4.0 | 31.5 | D:Optical.,SB:46.817d, e 0.692, K(A) 48.8 k/s, K(B) 48.7 k/s, V0 -5.1 k/s, m(A)sin3i = m(B)sin3i = 0.85,,SB:a(A)sini 22.7, a(B)sini 22.6.,VAR:BY Dra type predicted, but variability not yet detected. | |||||
HR 7581 | ι | CD-4214549 | 188114 | 229927 | 1520 | 19 55 15.7 | -41 52 06 | 4.13 | K0II-III | ||||||||
HR 7585 | CD-3314560 | 188158 | 211653 | 19 55 05.1 | -33 02 47 | 6.46 | K2/3III | ||||||||||
HR 7597 | ω | 58 | CD-2614637 | 188376 | 188722 | I | 19 55 50.4 | -26 17 58 | 4.70 | G5V | N:Terebellum, name shared with HR 7604, 7618, 7650. | ||||||
HR 7604 | 59 | CD-2714399 | 188603 | 188742 | I | 19 56 56.8 | -27 10 12 | 4.52 | K2.5IIb | N:Terebellum, name shared with HR 7597, 7618, 7650. | |||||||
HR 7605 | CD-3813776 | 188642 | 211686 | 19 57 41.3 | -38 03 30 | 6.55 | F4V | ||||||||||
HR 7614 | 61 | BD-15 5516 | 188899 | 163141 | 1522 | 19 57 57.0 | -15 29 29 | 5.02 | A3IV | ||||||||
HR 7617 | CD-3017525 | 188981 | 211708 | 19 58 56.4 | -30 32 17 | 6.28 | K1III | ||||||||||
HR 7618 | 60 | CD-2614682 | 189005 | 188778 | I | 19 58 57.2 | -26 11 44 | 4.83 | G6IIIBa0.2 | N:See HR 7597. | |||||||
HR 7623 | θ1 | CD-3513831 | 189103 | 211716 | 751 | 19 59 44.2 | -35 16 35 | 4.37 | B3IV | G:Member of the local association (Pleiades group).,SB:2.1051d, K 15.9k/s, V0 +0.9k/s, asini 0.460. | |||||||
HR 7624 | θ2 | CD-3513832 | 189118 | 211717 | W | 19 59 51.3 | -34 41 52 | 5.30 | A4/5IV | 5.5 | 30. | ||||||
HR 7627 | CD-4313735 | 189140 | 229977 | 20 00 26.5 | -43 02 36 | 6.14 | M0II-III | ||||||||||
HR 7629 | CD-3813802 | 189195 | 211719 | W | 20 00 15.9 | -37 42 08 | 5.95 | G8III | 7.6 | 23.0 | |||||||
HR 7630 | CD-4513549 | 189198 | 229981 | 3597 | 20 00 48.3 | -45 06 47 | 5.81 | A8III | S:Also classified F0/2IV. | ||||||||
HR 7631 | CD-3414082 | 189245 | 211724 | 12655 | 20 00 20.3 | -33 42 14 | 5.66 | F7V | SB:Unresolved by speckle interferometry 1986.46.,VAR:Amp. 0.07V. | ||||||||
HR 7639 | CD-4113807 | 189388 | 229993 | 20 01 26.4 | -40 48 51 | 6.29 | A2-3V | ||||||||||
HR 7643 | CD-2315935 | 189561 | 188829 | 3600 | 20 01 23.9 | -22 44 14 | 6.01 | G7V | |||||||||
HR 7649 | 63 | BD-14 5618 | 189741 | 163195 | 20 01 58.6 | -13 38 13 | 5.71 | A3V | |||||||||
HR 7650 | 62 | CD-2816355 | 189763 | 188844 | 753 | I | V3872 Sgr | 20 02 39.5 | -27 42 35 | 4.58 | M4III | C:May not be the IR source.,N:See HR 7597.,VAR:L? 4.45 - 4.61V. | |||||
HR 7652 | CD-3813828 | 189831 | 211767 | 3602 | 20 03 33.5 | -37 56 27 | 4.77 | K5III | G:Hyades group; Zeta Her group. | ||||||||
HR 7658 | BD-22 5318 | 190009 | 188863 | D | 20 03 44.3 | -22 35 44 | 6.45 | F6V | D:Suspected occultation double. | ||||||||
HR 7659 | CD-3215682 | 190056 | 211782 | 3606 | I | W | 12746 | 20 04 19.6 | -32 03 23 | 4.99 | K1III | 7.6 | 51.3 | ||||
HR 7668 | CD-3314700 | 190306 | 211798 | W | 20 05 32.1 | -33 00 00 | 6.53 | B8 | 1.0 | 0.4 | |||||||
HR 7675 | 65 | BD-13 5569 | 190454 | 163253 | 20 05 26.4 | -12 39 55 | 6.55 | A1Vn | |||||||||
HR 7703 | CD-3613940 | 191408 | 211885 | W | 20 11 11.9 | -36 06 04 | 5.32 | K3V | 4.0 | D:AB CPM. B, 11v dM5, sep. 6.6". Wroclaw contr. no. 16 gives mag. differences but no sep. for four components: AB 5.4v,,D:AC 5.15, and AD 4.0. Possible misidentification? Discovered by John Herschel as simply double. Components C and D,D:apparently first listed by van Albada at Lembang in 1958; only magnitudes and no separations were indicated. | |||||||
HR 7706 | CD-4313855 | 191584 | 230100 | 20 12 23.9 | -42 46 50 | 6.22 | K1III | ||||||||||
HR 7725 | CD-3017773 | 192433 | 211940 | 3621 | 20 15 50.6 | -30 00 19 | 6.30 | K4III | |||||||||
HR 7728 | CD-3614011 | 192472 | 211948 | W | 12949 | 20 16 23.7 | -36 27 16 | 6.39 | M4III | 5.1 | 38.0 | ||||||
HR 7729 | CD-3514020 | 192486 | 211950 | 20 16 26.5 | -35 11 52 | 6.53 | F2V | ||||||||||
HR 7764 | CD-2916981 | 193281 | 189164 | 13702 | 20 20 28.1 | -29 11 50 | 6.30 | A4/7V | 1.1 | 27.2 | C:Combined mag. and color of AB and C.,D:Component C, photometric spectral class A2IV, vsini 53k/s. Component B, 10.1V at 4.1". For component AB, Rakos and,D:Mermilliod give 6.93V, +0.28(B-V), +0.24(U-B). However, other sources give the following V magnitudes:,D:Comp. 1976 1978 1980 Preferred,D:Gronbech and Oblak Ruffener,D:Olsen,D:AB 6.635 6.610 6.608 6.61,D:C 7.724 7.706 7.72,D:Colors converted from the uvby system (Gronbech and Olsen) are AB +0.13(B-V), +0.185(U-B); C +0.165(B-V), +0.14(U-B).,S:Photometric spectral class A2III. | ||||||
HR 7765 | CD-3614057 | 193302 | 212025 | 1530 | 20 20 51.9 | -35 40 25 | 6.46 | K3-4III | |||||||||
HR 7779 | κ1 | CD-4214836 | 193571 | 230177 | 763 | W | 20 22 27.5 | -42 02 59 | 5.59 | A0V | 6.0 | 52.0 | |||||
HR 7787 | κ2 | CD-4214847 | 193807 | 230184 | W | 20 23 53.2 | -42 25 22 | 5.64 | A5V | 0.9 | 0.6 | D:AB binary. Combined mag., colors.,DYN:0.011". | |||||
HR 7799 | CD-4114024 | 194184 | 230197 | 20 25 47.9 | -40 47 47 | 6.09 | K3III | SB:117.776d, K 22.6k/s, V0 +42.1k/s, asini 35.5. | |||||||||
HR 7801 | CD-2917049 | 194215 | 189264 | 1532 | D | 20 25 26.8 | -28 39 48 | 5.85 | G8II/III | SB:377.60d, K 11.2k/s, V0 -7.3k/s, asini 58.0. | |||||||
HR 7808 | CD-3713741 | 194433 | 212126 | W | 20 26 53.0 | -37 24 11 | 6.25 | K2IV-V | 1.4 | 1.1 | D:6.6 K2IV-V, 7.8 K1V, 232.76y, a = 1.225".,DYN:0.024". |
Planetarische Nebel | ||||||||
---|---|---|---|---|---|---|---|---|
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 6439 | 17 48 19.8 | -16 28 44 | PN | 13.8 | 12.6 | 0.23 | planetary, stellar = 13 m | PK 11+5.1, CS=18.5 |
NGC 6445 | 17 49 15.1 | -20 00 32 | PN | 13.2 | 11.2 | 0.73 | pB, pS, R, gbM, r, * 15 np | PK 8+3.1, ESO 589-PN9, CS=19.1, Little Gem nebula |
NGC 6537 | 18 05 13.0 | -19 50 32 | PN | 12.5 | 11.6 | 0.17 | planetary, B, S, stellar | PK 10+0.1, ESO 590-PN1, CS=19.5 |
NGC 6563 | 18 12 02.6 | -33 52 04 | PN | 13.8 | 11.0 | 0.8 | planetary, F, L, cE, hazy border | PK 358-7.1, ESO 394-PN33, CS=18.3 |
NGC 6565 | 18 11 52.5 | -28 10 41 | PN | 13.2 | 11.6 | 0.23 | planetary, stellar | PK 3-4.5, ESO 456-PN70, CS=19.5 |
NGC 6567 | 18 13 45.1 | -19 04 32 | PN | 11.7 | 11.0 | 0.2 | planetary, stell, 11 mag, in a Cl | PK 11-0.2, ESO 590-PN8, CS=15.0 |
NGC 6578 | 18 16 16.5 | -20 27 00 | PN | 13.1 | 12.9 | 0.18 | planetary, stellar = 13 mag | PK 10-1.1, ESO 590-PN12, CS=11.8 |
NGC 6620 | 18 22 54.2 | -26 49 16 | PN | 15.0 | 12.7 | 0.13 | planetary, stellar | PK 5-6.1, ESO 522-PN22 |
NGC 6629 | 18 25 42.4 | -23 12 08 | PN | 11.6 | 11.3 | 0.27 | planetary or globular, pB, eeS, R | PK 9-5.1, ESO 522-PN26, CS=12.8 |
NGC 6644 | 18 32 34.7 | -25 07 42 | PN | 12.2 | 10.7 | 0.2 | planetary, stellar | PK 8-7.2, ESO 522-PN33, CS=15.9 |
NGC 6818 | 19 43 57.8 | -14 09 09 | PN | 9.9 | 9.3 | 0.77 | planetary, B, vS, R | PK 25-17.1, CS=16.1 |
IC 4670 | 17 55 07.0 | -21 44 39 | PN | 13.1 | 12.0 | 0.08 | stellar, 12.5 magn | PK 7+1.1, CS=15.0 |
IC 4673 | 18 03 18.4 | -27 06 22 | PN | 12.9 | 13.0 | 0.25 | Planetary, 13 mag, * 13 nf 33" | PK 3-2.3, ESO 521-PN15, CS=14.6 |
IC 4732 | 18 33 54.6 | -22 38 39 | PN | 13.3 | 12.1 | 0.22 | Planetary, stellar | PK 10-6.1, ESO 523-PN1, CS>16.6 |
IC 4776 | 18 45 50.7 | -33 20 32 | PN | 11.7 | 10.8 | 0.3 | Planetary, stellar | PK 2-13.1, ESO 396-PN2, CS>14.6 |
Galaktische Nebel | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 6514 | 18 02 42.0 | -22 58 18 | EN+OCL | 8.5 | 20 × 20 | !!! vB, vL, trifid, D * inv | M 20, OCL 23, ESO 521-N*13, LBN 27, Trifid nebula | |
NGC 6523 | 18 03 42.0 | -24 22 48 | EN | 5.8 | 45 × 30 | !!! vB, eL, eiF, with L Cl | M 8, NGC 6533, LBN 25, Lagoon nebula | |
NGC 6559 | 18 09 57.6 | -24 06 35 | EN | 8 × 5 | vF, vL, lE, ** inv | LBN 29, ESO 521-*N40, Sh2-29 | ||
NGC 6589 | 18 16 51.7 | -19 46 41 | RN | 5 × 3 | D * in centre of eF, pL neby | IC 4690, LBN 46, ESO 590-N14 | ||
NGC 6595 | 18 17 04.8 | -19 51 58 | EN+OCL | 7.0 | 11 | F, pL, cE, ** inv | NGC 6590, IC 4700, ESO 590-SC15, OCL 31, CED 157B, LBN 43, DG 150 | |
NGC 6618 | 18 20 47.0 | -16 10 18 | EN+OCL | 6.0 | 20 × 15 | !!!, B, eL, eiF, 2 hooked | M 17, OCL 44, LBN 60, Sh2-45, Omega nebula | |
IC 1271 | 18 05 13.0 | -24 24 38 | EN+* | eF, vL, B * inv | ESO 521-*N22, LBN 26 ? | |||
IC 1274 | 18 09 50.0 | -23 38 54 | EN+* | 6 × 5 | 3 st 8.5 to 9m in pL neb | LBN 33, ESO 521-N*41, CED 154D, Sh2-31 | ||
IC 1275 | 18 10 07.0 | -23 45 42 | EN+* | 2 st 8 & 8.5 in pL neb | ||||
IC 1283 | 18 17 16.7 | -19 45 44 | EN | 3 × 3 | * 9.3 nebulous | in Sh2-37, part of IC 1284 | ||
IC 1284 | 18 17 39.5 | -19 40 19 | EN+* | 17 × 15 | * 7.6 in neb, 15' diam | ESO 590-*N16, CED 157D, in Sh2-37 | ||
IC 4678 | 18 06 33.4 | -23 57 16 | EN+* | B, S, E | ESO 521-N*26, CED 152B, NE of Lagoon nebula (M 8) | |||
IC 4684 | 18 09 08.6 | -23 26 09 | EN+* | 3 × 2 | S neb or neb * | LBN 34, ESO 521-N*33 | ||
IC 4701 | 18 16 00.0 | -16 38 00 | EN | 60 × 40 | eL, conn with cloud I.C. 4715 | LBN 56, COU 25 | ||
IC 4706 | 18 19 36.0 | -16 01 54 | EN | 5 × 5 | * 9.2 in S neb, conn with M 17 | CED 160A | ||
IC 4707 | 18 19 54.0 | -16 00 06 | EN | 3.5 × 3.5 | * 9.4 in S neb, conn with M 17 | CED 160B | ||
Offene Sternhaufen | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 6469 | 17 52 56.5 | -22 18 43 | III2p | 8.2 | 8 | Cl, pRi (in M Way) | OCL 21, ESO 589-SC18 | |
NGC 6494 | 17 56 56.0 | -19 00 42 | III1m | 5.5 | 25 | Cl, B, vL, pRi, lC, st 10… | M 23, OCL 30, ESO 589-SC22 | |
NGC 6506 | 17 59 53.4 | -24 41 07 | III2p | Cl, Ri, eL, vlC | OCL 16, ESO 521-SC6 | |||
NGC 6507 | 17 59 50.0 | -17 27 00 | IV2p | 9.6 | 7 | Cl, pS, lRi, lC | OCL 32 | |
NGC 6520 | 18 03 25.0 | -27 53 28 | I2m | 7.6 | 5 | Cl, pS, Ri, lC, st 9…13 | OCL 10, ESO 456-SC42 | |
NGC 6530 | 18 04 30.0 | -24 21 30 | II2mn | 4.6 | 15 | Cl, B, L, pRi, f M 8 | OCL 19, ESO 521-SC21, in Lagoon nebula (M 8) | |
NGC 6531 | 18 04 13.3 | -22 30 00 | I3m | 5.9 | 16 | Cl, pRi, lC, st 9…12 | M 21, OCL 26, ESO 521-SC19 | |
NGC 6546 | 18 07 22.0 | -23 17 48 | III2m | 8.0 | 15 | Cl, vL, vRi | OCL 24, ESO 521-SC29 | |
NGC 6568 | 18 12 44.0 | -21 35 00 | III1m | 8.6 | 12 | Cl, vL, lC | OCL 28, ESO 590-SC6 | |
NGC 6583 | 18 15 48.8 | -22 08 15 | II1m | 10.0 | 5 | Cl, pRi, pC, cE, st 13… | OCL 27, ESO 590-SC11 | |
NGC 6596 | 18 17 33.0 | -16 39 00 | III2m | 10 | Cl, lC | OCL 41 | ||
NGC 6603 | 18 18 24.0 | -18 24 24 | I1r | 11.1 | 4 | !, Cl, vRi, vmC, R, st 15 (M Way) | OCL 36, ESO 590-SC17, in M 24 | |
NGC 6613 | 18 19 58.0 | -17 06 06 | II3pn | 6.9 | 7 | Cl, P, vlC | M 18, OCL 40 | |
NGC 6645 | 18 32 37.8 | -16 53 02 | III1m | 8.5 | 15 | Cl, pL, vRi, pC, st 11…15 | OCL 48 | |
NGC 6647 | 18 32 49.0 | -17 13 42 | OCL | 8.0 | Cl, L, Ri, lC, st vS | |||
NGC 6716 | 18 54 34.0 | -19 54 30 | IV1p | 7.5 | 10 | Cl, pRi, st 9…13 | OCL 46, ESO 592-SC5 | |
NGC 6774 | 19 16 18.0 | -16 19 30 | III2m | 20 | Cl, vL, lC | OCL 65, Ruprecht 147 | ||
IC 4685 | 18 09 17.4 | -23 59 14 | IV3pn | 15 × 10 | * 7.5 in L, dif neb | OCL 22, ESO 521-*N37, a x b of nebula | ||
IC 4715 | 18 18 48.0 | -18 33 00 | *Cloud | eeL cloud of st and neb | M 24, ESO 591-**1, Sagittarius Star Cloud | |||
IC 4725 | 18 31 45.0 | -19 07 12 | I2p | 4.6 | 26 | Cl, pC | M 25, OCL 38, ESO 591-SC6 | |
Kugelsternhaufen | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 6440 | 17 48 52.6 | -20 21 32 | V | 9.3 | 4.4 | pB, pL, R, bM | GCL 77, ESO 589-SC8 | |
NGC 6522 | 18 03 34.1 | -30 02 00 | VI | 9.9 | 9.4 | globular, B, pL, R, gvmbM, rrr, st 16 | GCL 82, ESO 456-SC43 | |
NGC 6528 | 18 04 49.6 | -30 03 19 | V | 9.6 | 5 | globular, pF, cS, R, gbM, rrr, st 16 | GCL 84, ESO 456-SC48 | |
NGC 6540 | 18 06 08.6 | -27 45 53 | GCL | 9.3 | 1.5 | pF, S, iE, er or Cl | OCL 11, ESO 456-SC53, Djorgovsky 3 | |
NGC 6544 | 18 07 20.6 | -24 59 49 | V | 7.5 | 9.2 | cF, pL, iR, r | GCL 87, ESO 521-SC28 | |
NGC 6553 | 18 09 15.6 | -25 54 26 | XI | 8.3 | 9.2 | globular, F, L, lE, vglbM, rr, st 20 | GCL 88, ESO 521-SC36 | |
NGC 6558 | 18 10 18.4 | -31 45 47 | GCL | 8.6 | 4.2 | globular, pB, pL, R, glbM, rrr, st 16 | GCL 89, ESO 456-SC62 | |
NGC 6569 | 18 13 38.9 | -31 49 33 | VIII | 8.4 | 6.4 | globular, cB, L, R, rrr, st 15… | GCL 91, ESO 456-SC77 | |
NGC 6624 | 18 23 40.5 | -30 21 38 | VI | 7.6 | 8.8 | globular, vB, pL, R, rrr, st 16 | GCL 93, ESO 457-SC11 | |
NGC 6626 | 18 24 32.9 | -24 52 10 | IV | 6.9 | 13.8 | !, globular, vB, L, R, geCM, rrr, st 14…16 | M 28, GCL 94, ESO 522-SC23 | |
NGC 6637 | 18 31 23.2 | -32 20 51 | V | 9.3 | 8.3 | 7.1 | globular, B, L, R, rrr, st 14…16 | M 69, GCL 69, ESO 457-SC14 |
NGC 6638 | 18 30 56.2 | -25 29 45 | VI | 9.2 | 7.3 | globular, B, S, R, rr | GCL 95, ESO 522-SC30 | |
NGC 6642 | 18 31 54.3 | -23 28 33 | IV | 8.9 | 5.8 | globular, pB, pL, iR, gpmbM, rrr, st 16 | GCL 97, ESO 522-SC32 | |
NGC 6652 | 18 35 45.7 | -32 59 23 | VI | 8.5 | 6 | B, S, lE, rrr, st 15 | GCL 98, ESO 395-SC11 | |
NGC 6656 | 18 36 24.2 | -23 54 10 | VII | 5.2 | 32 | !!, globular, vB, vL, R, vRi, vmC, st 11…15 | M 22, GCL 99, ESO 523-SC4 | |
NGC 6681 | 18 43 12.7 | -32 17 29 | V | 7.8 | 8 | globular, B, pL, R, gbM, st 14…17 | M 70, GCL 101, ESO 458-SC3 | |
NGC 6715 | 18 55 03.3 | -30 28 40 | III | 7.7 | 12 | globular, vB, L, R, g, smbM, rrr, st 15 | M 54, GCL 104, ESO 458-SC8 | |
NGC 6717 | 18 55 06.2 | -22 42 01 | VIII | 8.4 | 5.4 | F, S, rr, Cl + neb | Pal 9, GCL 105, ESO 523-SC14 | |
NGC 6723 | 18 59 33.2 | -36 37 52 | VII | 6.8 | 13 | globular, vL, vlE, vgbM, rrr, st 14…16 | GCL 106, ESO 396-SC10 | |
NGC 6809 | 19 39 59.4 | -30 57 42 | XI | 6.3 | 19 | globular, pB, L, R, vRi, vgbM, st 12…15 | M 55, GCL 113, ESO 460-SC21 | |
NGC 6864 | 20 06 04.8 | -21 55 15 | I | 8.6 | 6.8 | globular, B, pL, R, vmbMBN, rr | M 75, GCL 116, ESO 595-SC13 | |
Galaxien | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 6794 | 19 28 03.8 | -38 55 07 | Sab | 13.9 | 12.9 | 1.7 × 1.4 | eF, pS, R, vgvlbM | ESO 338-5, MCG -7-40-1 |
NGC 6805 | 19 36 45.8 | -37 33 14 | E1 | 13.8 | 12.8 | 1.1 × 0.9 | eF, R, vgbM | ESO 338-14, MCG -6-43-2 |
NGC 6806 | 19 37 04.8 | -42 17 45 | SBc | 13.7 | 13.2 | 1.2 × 0.8 | eF, vS, * 14 att | ESO 338-15, MCG -7-40-3, FAIR 1162, IRAS 19336-4224, VV 411, AM 1933-422 |
NGC 6816 | 19 44 02.4 | -28 24 03 | E-S0 | 14.1 | 12.9 | 1.2 × 0.8 | eF, pS, R, vlbM, * np | ESO 460-30, MCG -5-46-6 |
NGC 6822 | 19 44 56.6 | -14 48 23 | IBm | 9.3 | 8.7 | 15.4 × 14.2 | vF, L, E, dif | IC 4895, MCG -2-50-6, DDO 209, IRAS 19421-1455, Barnard's galaxy |
NGC 6835 | 19 54 32.8 | -12 34 03 | SBa | 13.4 | 12.5 | 2.4 × 0.7 | F, pL, mE | MCG -2-50-9, IRAS 19517-1241 |
NGC 6836 | 19 54 40.3 | -12 41 18 | SBm | 13.4 | 12.9 | 1.7 × 1.5 | vF, pL, R, dif | MCG -2-50-10, IRAS 19518-1249 |
NGC 6841 | 19 57 49.1 | -31 48 39 | E1 | 13.8 | 12.7 | 1.5 × 1.4 | vF, S, R, psbM | ESO 461-23, MCG -5-47-11 |
NGC 6849 | 20 06 15.6 | -40 11 54 | E/SB0 | 13.0 | 12.1 | 1.9 × 1.1 | pB, S, R, vS * np | ESO 339-32, MCG -7-41-7 |
NGC 6878 | 20 13 53.2 | -44 31 36 | SBb | 13.5 | 12.7 | 1.6 × 1.3 | vF, pL, R, glbM | ESO 284-31, MCG -7-41-15, IRAS 20104-4440 |
NGC 6878 A | 20 13 36.1 | -44 48 59 | SBb | 13.8 | 13.2 | 1.8 × 0.8 | vF, pL, R, glbM | ESO 284-29, MCG -7-41-13 |
NGC 6890 | 20 18 18.0 | -44 48 23 | SBb | 13.0 | 12.3 | 1.6 × 1.3 | pF, S, R, vglbM | ESO 284-54, MCG -7-41-23, IRAS 20148-4457 |
NGC 6902 | 20 24 27.9 | -43 39 11 | SBa | 11.6 | 10.9 | 5.6 × 3.9 | F, cS, R, bM | IC 4948, ESO 285-8, MCG -7-42-2, AM 2021-434 |
NGC 6902 A1 | 20 23 00.4 | -44 16 14 | SBm | 14.4 | 13.8 | 1.3 × 1 | F, cS, R, bM | ESO 285-4, MCG -7-41-32, AM 2019-442 |
NGC 6902 A2 | 20 22 58.8 | -44 16 22 | SB0 | 15.8 | 14.8 | 0.6 × 0.5 | F, cS, R, bM | ESO 285-4A, MCG -7-41-32, AM 2019-442 |
NGC 6902 B | 20 23 06.8 | -43 52 08 | SBcd | 14.1 | 13.6 | 1.5 × 1.2 | F, cS, R, bM | ESO 285-5, MCG -7-41-33, AM 2019-442 |
IC 1309 | 20 03 01.4 | -17 13 57 | SBbc | 15.0 | 14.2 | 0.9 × 0.7 | F, vS, R, r | |
IC 4816 | 19 01 44.4 | -13 08 50 | S | 17.0 | 16.2 | 0.2 × 0.1 | Planetary, stellar | |
IC 4913 | 19 56 47.5 | -37 19 43 | E-S0 | 14.0 | 13.0 | 1.1 × 0.7 | eeF, pS, e diffic, 3 st 10 s 8' | ESO 399-5, MCG -6-43-13 |
IC 4926 | 20 00 12.2 | -38 34 41 | E2 | 13.7 | 12.7 | 1.2 × 1 | eeF, S, lE, v diffic, p of 2 | ESO 339-18, MCG -6-44-5 |
IC 4931 | 20 00 50.1 | -38 34 30 | E2 | 13.0 | 11.8 | 2.4 × 2 | eeF, pS, R, * 8 f 20s, f of 2 | ESO 339-23, MCG -6-44-8 |
IC 4946 | 20 23 58.0 | -43 59 43 | SB0-a | 12.6 | 11.8 | 2.4 × 1 | eF, S, R | ESO 285-7, MCG -7-42-1, A 2020-44, New 5 |
IC 4998 | 20 22 10.6 | -38 18 31 | SBc | 13.9 | 13.2 | 1.6 × 1.2 | eF, pS, R, bet 2 st 8.5 sp, nf | IC 5018, ESO 340-20, MCG -6-44-30, IRAS 20188-3828 |
PNG | RA | Dec | Main ID | PK | IRAS | Discoverer | Identities | oDiam ["] | rDiam ["] | Dist [kpc] | Rvel [km/s] | ExpVel [km/s] | C* Name | C* Mag | C* SP Type |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
PN G000.0-06.8 | 18 13 18 | -32 19 43 | H 1-62 | 359-06.1 | 18100-3220 | HARO 1952 | AS 290, ESO 456-76, He 2-367, MHa 77- 52, SaSt 2-19, VV' 368, Wray 16-389 | 0. | -84.0 ± 5.0 | B: 15.09, V: 14.92 | |||||
PN G000.1-01.1 | 17 50 24 | -29 25 18 | M 3-43 | 0-01.1 | 17472-2924 | MINKOWSKI 1948 | Bl G, ESO 455-48, VV' 265, 19W122 | 3.6 | +20.0 ± 11.0 | AG82 267 | B: >21. | ||||
PN G000.1-02.3 | 17 55 21 | -29 58 02 | Bl 3-10 | 0-02.2 | 17519-2957 | BLANCO 1964 | ESO 456-16, Sa 2-265 | 9.0 | |||||||
PN G000.1-05.6 | 18 08 25 | -31 37 24 | H 2-40 | 0-05.1 | HARO 1952 | ESO 456-59, Sa 3-120, VV' 351, Wray 16- 374 | 12.4 | AG82 287 | B: >21. | ||||||
PN G000.2-01.9 | 17 53 46 | -29 43 46 | M 2-19 | 0-01.5 | 17505-2943 | MINKOWSKI 1947 | Bl N, ESO 456-07, He 2- 302, Sa 3- 88, VV 125, VV' 279, Wray 16- 325 | 8.2 | 5. | -45.0 ± 11.0 | V: 17.3 | ||||
PN G000.2-04.6 | 18 04 44 | -31 02 50 | Wray 16-363 | WRAY 1966 | Sa 3-117 | 6.4 | |||||||||
PN G000.3-04.6 | 18 05 02 | -30 58 15 | M 2-28 | 0-04.1 | 18018-3058 | MINKOWSKI 1947 | ESO 456-49, He 2- 338, Sa 2-293, VV 144, VV' 336, Wray 16- 366 | 4.8 | -17.0 ± 11.0 | ||||||
PN G000.4-01.9 | 17 54 25 | -29 36 09 | M 2-20 | 0-01.6 | 17512-2935 | MINKOWSKI 1947 | Bl P, ESO 456-12, He 2- 304, Sa 2-262, VV 127, VV' 282, Wray 16- 326 | 6.6 | 16.4 | +75.0 ± 11.0 | AG82 270 | V: 16.1 | WC 5-6, WC | ||
PN G000.4-02.9 | 17 58 19 | -30 00 41 | M 3-19 | 0-02.6 | 17551-3000 | MINKOWSKI 1948 | ESO 456-26, Sa 3-103, VV' 301, Wray 16- 339 | 5.7 | 7. | +158.0 ± 11.0 | V: 16.9 | ||||
PN G000.5-01.6 | 17 53 25 | -29 17 07 | Al 2-Q | 17502-2916 | ALLEN 1979 | 0. | -67.0 | ||||||||
PN G000.6-01.3 | 17 52 35 | -29 06 33 | Bl 3-15 | 0-01.2 | BLANCO 1964 | ESO 455-58 | 3.0 | ||||||||
PN G000.6-02.3 | 17 56 24 | -29 38 05 | H 2-32 | 0-02.3 | HARO 1952 | Bl 3-12, ESO 456-20, Sa 3-98, VV' 290, Wra 16-232 | 0. | +145.0 ± 11.0 | |||||||
PN G000.7-02.7 | 17 58 10 | -29 44 21 | M 2-21 | 0-02.4 | 17548-2944 | MINKOWSKI 1947 | ESO 456-24, He 2- 315, Sa 2-271, VV 131, VV' 300, Wray 16- 337 | 7.2 | -138.5 ± 12.5 | B: 15.8, V: 14.7 | |||||
PN G000.7-03.7 | 18 02 19 | -30 14 21 | M 3-22 | 0-03.1 | 17590-3014 | MINKOWSKI 1948 | ESO 456-39, H 1-48, Sa 2-283, VV' 320 | 7.3 | -54.0 ± 5.0 | B: 18.2, V: >17.8 | |||||
PN G000.7-07.4 | 18 17 37 | -31 56 35 | M 2-35 | 0-07.1 | 18143-3158 | MINKOWSKI 1947 | ESO 457-04, He 2- 384, Sa 2-324, StWr 2-16, VV 168, VV' 384, Wray 16- 403 | 5. : | -21.0 ± 11.0 | ||||||
PN G000.8-01.5 | 17 53 51 | -28 59 22 | Bl O | 0-01.3 | 17506-2858 | BLANCO 1961 | ESO 456-11, Sa 3- 90 | 0. | V: 17.6 | ||||||
PN G000.8-07.6 | 18 18 37 | -31 54 52 | H 2-46 | 0-07.2 | 18152-3156 | HARO 1952 | ESO 457-07, Sa 2-327, VV' 388 | 4. : | |||||||
PN G000.9-02.0 | 17 56 02 | -29 11 17 | Bl 3-13 | 0-02.1 | 17528-2910 | BLANCO 1964 | ESO 456-18, Sa 3- 94, Wray 16- 329 | 5.2 | 270. ± 80. | B: 17.0, V: 16.2 | |||||
PN G000.9-04.8 | 18 07 05 | -30 34 12 | M 3-23 | 0-04.2 | 18038-3034 | MINKOWSKI 1948 | ESO 456-54, He 2- 348, Sa 2-297, VV' 346, Wray 16- 370 | 11.4 | 12. | -156.0 ± 5.0 | |||||
PN G001.0-02.6 | 17 58 25 | -29 20 50 | Sa 3-104 | 17552-2920 | SANDULEAK 1976 | 5.2 | |||||||||
PN G001.1-01.6 | 17 54 52 | -28 48 55 | Sa 3- 92 | SANDULEAK 1976 | Al 2-S = PK 1-01 5 | 6.0 | |||||||||
PN G001.2-03.0 | 18 00 38 | -29 21 51 | H 1-47 | 1-03.1 | 17574-2921 | HARO 1952 | ESO 456-35, He 2- 323, VV' 312, Wray 16- 347 | < 5. | 2.5 | +109.2 ± 4.3 | B: 16.8, V: 16.2 | ||||
PN G001.2-03.9 | 18 03 54 | -29 51 26 | ShWi 2-5 | SHAW et al 1985 | KFL 5 | 4.0 | B: 18.5, V: 16.5 | ||||||||
PN G001.3-01.2 | 17 53 47 | -28 27 16 | Bl M | 1-01.1 | 17506-2826 | BLANCO 1961 | ESO 456-10, Sa 3- 89, Wray 17- 101 | 4.2 | 4.5 | ||||||
PN G001.4-03.4 | 18 02 27 | -29 25 08 | ShWi 2-1 | SHAW et al 1985 | 13. | -117.0 | B: 16.1, V: 15.8 | ||||||||
PN G001.5-06.7 | 18 16 12 | -30 52 08 | SwSt 1 | 1-06.2 | 18129-3053 | SWINGS et al 1940 | AS 295B, ESO 457-02, He 2-377, Sa 2-319, VV 164, VV' 378, Wray 16-397 | < 5. | 1.3 | -18.6 ± 2.6 | 13.0 (O-III), 14.5 (N-II) | AG82 300, CD -30 15469, CPD -30 5412, HD 167362, MWC 288 | B: 11.77, V: 11.76 | WC 9, Of-WR(C) | |
PN G001.6-01.3 | 17 54 35 | -28 12 43 | Bl Q | 1-01.2 | 17513-2812 | BLANCO 1961 | ESO 456-14, Sa 3- 91, Wray 17- 102 | 4.5 | |||||||
PN G001.7-01.6 | 17 56 03 | -28 14 12 | H 2-31 | 1-01.3 | HARO 1952 | ESO 456-19, Sa 3- 95, VV' 288 | 0. | ||||||||
PN G001.7-04.4 | 18 07 15 | -29 41 24 | H 1-55 | 1-04.1 | HARO 1952 | ESO 456-56, He 2- 347, VV' 345, Wray 16- 373 | < 5. | 2.5 | -52.0 ± 11.0 | B: 17.03, V: 16.57 | |||||
PN G001.7-04.6 | 18 07 54 | -29 44 35 | H 1-56 | 1-04.2 | 18047-2945 | HARO 1952 | ESO 456-57, He 3-1592, Sa 2-299, VV' 347 | 3. | 2.5 | -106.0 ± 11.0 | B: 16.6, V: 17.0 | ||||
PN G001.8-03.8 | 18 05 04 | -29 19 27 | ShWi 2-7 | SHAW et al 1985 | 12. | B: 15.54, V: 14.74 | |||||||||
PN G002.0-02.0 | 17 58 22 | -28 14 50 | H 1-45 | 2-02.1 | 17552-2814 | HARO 1952 | ESO 456-27, He 2- 317, Sa 2-272, VV' 303, Wray 16- 340 | 6.0 | +4.0 ± 11.0 | V: 16.8 | |||||
PN G002.0-06.2 | 18 15 06 | -30 15 33 | M 2-33 | 2-06.1 | 18118-3016 | MINKOWSKI 1947 | ESO 456-80, He 2- 372, Sa 2-317, StWr 2-11, VV 162, VV' 375, Wray 16- 394 | 5.8 | 4. | -112.0 ± 11.0 | B: 14.4, V: 14.4 | ||||
PN G002.0-13.4 | 18 45 51 | -33 20 40 | IC 4776 | 2-13.1 | 18425-3323 | FLEMING 1896 | ARO 522, ESO 396-02, He 2- 421, Sa 2-363, StWr 2-23, VV 204, VV' 446, Wray 16- 418, Y-C 2- 27 | 7.5 | 1.6 | +18.9 ± 0.7 | 14.5 (N-II) | AG82 329, CD -33 13537, GCRV 11192, HD 173283 | B: 14.3, V: 14.1 | WC 6 ? | |
PN G002.1-02.2 | 17 59 19 | -28 13 48 | M 3-20 | 2-02.2 | 17561-2813 | MINKOWSKI 1948 | ESO 456-32, He 2- 319, Sa 2-276, VV' 307, Wray 16- 343 | 6.6 | +55.0 ± 11.0 | 23.5 (O-III) | |||||
PN G002.1-04.2 | 18 07 07 | -29 12 56 | H 1-54 | 2-04.1 | 18039-2913 | HARO 1952 | AS 272, ESO 456-55, He 2- 346, MHa 82- 21, Sa 2-298, VV' 344, Wray 16- 372 | 4.8 | 1.2 | -116.0 ± 11.0 | B: 15.7, V: 15.4 | ||||
PN G002.2+00.5 | 17 48 46 | -26 43 31 | Te 2337 | TERZAN 1989 | 28. | ||||||||||
PN G002.2-02.5 | 18 01 00 | -28 16 19 | KFL 2 | KINMAN et al 1988 | 5.4 | -101.0 | |||||||||
PN G002.2-02.7 | 18 01 43 | -28 25 45 | M 2-23 | 2-02.4 | 17585-2825 | MINKOWSKI 1947 | ESO 456-34, He 2- 326, My 112, Sa 2-281, VV 136, VV'316, Wray 16- 350 | 8.5 | 0.7 | +224.1 ± 10.1 | B: 16.7 | ||||
PN G002.2-06.3 | 18 16 19 | -30 07 36 | H 1-63 | 2-06.2 | 18131-3008 | HARO 1952 | ESO 457-03, He 2- 380, Sa 2-321, VV' 381, Wray 15-1853 | 7.0 | < 2.2 | -1.0 ± 11.0 | AG82 301 | B: 14.7, V: 14.7 | |||
PN G002.2-09.4 | 18 29 12 | -31 30 00 | Cn 1-5 | 2-09.1 | 18259-3132 | CANNON 1921 | Em 1, ESO 457-12, He 2- 402, Sa 2-337, StWr 2-17, Wray 16- 412 | 7. | 7. | -29.7 ± 4.0 | 18.0 (O-III) | AG82 312, CD -31 18259, CSI -31 18259, HD 170124 | B: 15.5, V: 15.2 | WC 4 | |
PN G002.3-03.4 | 18 04 28 | -28 37 41 | H 2-37 | 2-03.2 | HARO 1952 | ARO 268, ESO 456-46, Sa 2-291, VV' 333 | 4.2 | ||||||||
PN G002.3-07.8 | 18 22 34 | -30 43 29 | M 2-41 | 2-07.1 | 18194-3045 | MINKOWSKI 1947 | ESO 457-10, He 2- 392, Sa 2-330, StWr 2-13, VV 176, VV' 397, Wray 16- 408 | 14.2 | -82.0 ± 25.0 | ||||||
PN G002.4-03.2 | 18 04 05 | -28 27 55 | Wray 17-107 | WRAY 1966 | Sa 3-115 | 12. | |||||||||
PN G002.4-03.7 | 18 06 06 | -28 40 34 | M 1-38 | 2-03.5 | 18029-2840 | MINKOWSKI 1946 | ESO 456-52, He 2- 344, SaSt 2-18, VV 148, VV' 340, Wray 16- 368 | < 3.3 | 3.5 | -70.0 ± 11.0 | B: 14.90, V: 14.45 | ||||
PN G002.5-01.7 | 17 58 31 | -27 37 05 | Pe 2-11 | 2-01.1 | PEREK 1960 | ESO 456-30, Sa 3-106, VV' 305 | 5.1 | AG82 276 | B: >21. | ||||||
PN G002.5-05.4 | 18 13 00 | -29 25 12 | KFL 14 | KINMAN et al 1988 | 17.1 | +107.0 | B: 18.6, V: 17.7 | ||||||||
PN G002.6-03.4 | 18 05 26 | -28 22 04 | M 1-37 | 2-03.3 | 18022-2822 | MINKOWSKI 1946 | ESO 456-50, He 2- 339, VV 146, VV' 338, Wray 16- 367 | 0. | 2.5 | +241.0 ± 11.0 | B: 15.34, V: 14.99 | ||||
PN G002.7-04.8 | 18 11 05 | -28 59 01 | M 1-42 | 2-04.2 | 18079-2859 | MINKOWSKI 1946 | ESO 456-67, He 2- 359, Sa 2-305, StWr 2- 8, VV 153, VV' 357, Wray 16- 380 | 9.0 | 9.0 | -92.0 ± 3.0 | 25.0 (O-III), < 6.0 (N-II) | AG82 291 | B: 18.3, V: 17.4 | ||
PN G002.8-02.2 | 18 01 10 | -27 38 26 | Pe 2-12 | 2-02.3 | 17580-2738 | PEREK 1960 | ESO 456-36, Sa 3-110, VV' 314, Wray 17- 105 | 5. | |||||||
PN G002.9-03.9 | 18 08 04 | -28 23 32 | H 2-39 | 2-03.6 | HARO 1952 | ESO 456-58, Sa 2-301, VV' 350 | 3.7 | ||||||||
PN G003.0-02.6 | 18 02 51 | -27 41 02 | KFL 4 | KINMAN et al 1988 | 3.0 | +17.0 | |||||||||
PN G003.2-04.4 | 18 10 31 | -28 19 22 | KFL 12 | KINMAN et al 1988 | 2.8 | +124.0 | |||||||||
PN G003.2-06.2 | 18 17 42 | -29 08 20 | M 2-36 | 3-06.1 | 18144-2909 | MINKOWSKI 1947 | Em 5, ESO 457-05, He 2- 385, Sa 2- 325, StWr 2- 10, VV 169, VV' 385, Wray 16- 404 | 8.1 | +100.4 ± 10.1 | B: 15.47, V: 15.73 | |||||
PN G003.3-04.6 | 18 11 35 | -28 22 37 | Ap 1-12 | 3-04.7 | 18084-2823 | APRIAMASVILI 1961 | AS 283, ESO 456-69, He 2- 360, MHa 304-120, , Wray 16- 381 | 12. | +152.0 ± 5.0 | SS73 140 | B: 13.37, V: 13.29 | ||||
PN G003.3-07.5 | 18 23 09 | -29 43 25 | KFL 19 | KINMAN et al 1988 | 7.8 | +32.0 | |||||||||
PN G003.4-04.8 | 18 12 48 | -28 20 01 | H 2-43 | 3-04.9 | 18095-2820 | HARO 1952 | AS 288, ESO 456-75, He 2- 366, MHa 304-119, VV' 367, Wray 16- 388 | 9. | -21.0 ± 3.0 | ||||||
PN G003.5-02.4 | 18 03 18 | -27 06 16 | IC 4673 | 3-02.3 | 18001-2706 | BARNARD 1896 | ESO 521-15, He 2- 333, M 1-36, Sa 2- 286, VV 142, VV' 330, Wray 16- 357 | 14.8 | 17. | -15.0 ± 2.0 | 25.0 (O-III) | AG82 283 | B: 18.0, V: 17.6 | ||
PN G003.5-04.6 | 18 11 53 | -28 10 38 | NGC 6565 | 3-04.5 | 18087-2811 | PICKERING 1880 | ARO 68, BD -28 14266, ESO 456-70, GCRV 10632, He 2- 362, HD 166468, Sa 2-307, StWr 2- 9, VV 155, VV' 360, Wray 16-382 | 13.6 | 1.5 | 1.3 | -20.0 ± 4.0 | 14.5 (O-III), 22.0 (N-II) | AG82 292 | V: 18.50 | |
PN G003.6-02.3 | 18 03 12 | -26 58 31 | M 2-26 | 3-02.2 | 18001-2659 | MINKOWSKI 1947 | ESO 521-14, He 2- 332, Sa 3-113, VV 139, VV' 322, Wray 17- 106? | 9.2 | -52.0 ± 5.0 | AG82 281 | |||||
PN G003.7-04.6 | 18 12 34 | -27 58 13 | M 2-30 | 3-04.8 | 18094-2758 | MINKOWSKI 1947 | ESO 456-74, He 2- 365, VV 157, VV' 366, Sa 2-312, StWr 2- 7, Wray 16- 386 | 9.0 | 3.5 | +174.0 ± 11.0 | B: 17.7, V: 17.1 | ||||
PN G003.8-04.3 | 18 11 29 | -27 46 16 | H 1-59 | 3-04.3 | HARO 1952 | ESO 456-68, Sa 2-306, StWr 2- 6, VV' 356 | 6.0 | B: 18.2, V: 16.2 | |||||||
PN G003.8-04.5 | 18 12 24 | -27 52 14 | H 2-41 | 3-04.4 | 18092-2752 | HARO 1952 | ESO 456-71, Sa 2-309, VV' 363 | 8.1 | AG82 294 | ||||||
PN G003.8-17.1 | 19 05 36 | -33 11 39 | Hb 8 | 3-17.1 | 19022-3316 | HUBBLE 1921 | ESO 397-02, He 2- 426, Sa 2-381, StWr 2-24, VV 218, VV' 475, Y-C 2- 33 | 5. | 0.8 | -172.1 ± 7.7 | AG82 343 | ||||
PN G003.9+01.6 | 17 48 28 | -24 41 29 | Te 2111 | TERZAN 1989 | 8. | ||||||||||
PN G003.9-02.3 | 18 03 39 | -26 43 25 | M 1-35 | 3-02.1 | 18005-2643 | MINKOWSKI 1946 | ESO 521-17, He 2- 336, Sa 2-287, VV 141, VV' 328, Wray 15- 1830 | 4.5 | 4.4 | +82.0 ± 11.0 | |||||
PN G003.9-03.1 | 18 06 50 | -27 06 18 | KFL 7 | KINMAN et al 1988 | 5.0 | -91.0 | |||||||||
PN G003.9-14.9 | 18 55 39 | -32 15 55 | Hb 7 | 3-14.1 | 18523-3219 | HUBBLE 1921 | ARO 523, Cn 1-6, AS 330, ESO 458-09, He 2- 425, Sa 2-375, StWr 2-20, VV 212, VV' 463, Wray 16-422, Y-C 2- 31 | 4. | -65.4 ± 4.8 | AG82 335, CD -32 14673, GCRV 11357, HD 175194 | B: 13.90, V: 13.97 | O | |||
PN G004.0-03.0 | 18 06 42 | -26 55 21 | M 2-29 | 4-03.1 | 18035-2655 | MINKOWSKI 1947 | ESO 521-27, He 2- 345, Sa 2-296, VV 149, VV' 343, Wray 17- 109 | 3.6 | 3.5 | -114.0 ± 11.0 | B: 15.60, V: 15.54 | ||||
PN G004.0-05.8 | 18 17 42 | -28 17 19 | Pe 1-12 | 4-05.3 | PEREK 1960 | ESO 457-06, VV' 386 | 9.6 | B: 17.7, V: 17.2 | |||||||
PN G004.0-11.1 | 18 39 26 | -30 40 36 | M 3-29 | 4-11.1 | 18362-3043 | MINKOWSKI 1948 | Em 2, ESO 458-01, He 2- 416, Sa 2-355, StWr 2-14, VV' 434, Wray 16- 416 | 8.2 | +50.3 ± 5.4 | 7.0 (O-III) | AG82 323 | B: 15.42, V: 15.50 | |||
PN G004.1-03.8 | 18 10 12 | -27 16 36 | KFL 11 | KINMAN et al 1988 | 3.2 | -63.0 | |||||||||
PN G004.2-03.2 | 18 08 01 | -26 54 01 | KFL 10 | KINMAN et al 1988 | 6.0 | -121.0 | |||||||||
PN G004.2-04.3 | 18 12 25 | -27 28 55 | H 1-60 | 4-04.1 | HARO 1952 | ESO 522-03, Sa 2-310, VV' 362 | 5.7 | B: 16.7, V: 16.4 | WC ? | ||||||
PN G004.2-05.9 | 18 18 39 | -28 08 05 | M 2-37 | 4-05.5 | 18154-2809 | MINKOWSKI 1947 | ESO 457-08, He 2- 387, Sa 3-131, VV 170, VV' 390, Wray 15- 1858 | 7.2 | +57.0 ± 5.0 | B: 17.6, V: 16.8 | |||||
PN G004.3+01.8 | 17 48 36 | -24 16 36 | H 2-24 | 4+01.1 | HARO 1952 | ESO 520-29, Sa 3- 77, VV' 254 | 4.6 | ||||||||
PN G004.3-02.6 | 18 05 57 | -26 29 42 | H 1-53 | 4-02.1 | HARO 1952 | ARO 269, ESO 521-24, He 2- 342, VV' 341 | 0. | +75.0 ± 5.0 | |||||||
PN G004.7-11.8 | 18 44 13 | -30 18 27 | He 2-418 | 4-11.2 | HENIZE 1964 | ESO 458-04, Sa 2-360, StWr 2-15, Wray 16- 417 | 13. | B: 15.48, V: 15.68 | |||||||
PN G004.8+02.0 | 17 49 01 | -23 42 55 | H 2-25 | 4+02.1 | 17459-2342 | HARO 1952 | ESO 520-30, VV' 258 | 4.4 | 4.9 | ||||||
PN G004.8-05.0 | 18 16 11 | -27 14 57 | M 3-26 | 4-05.1 | 18130-2715 | MINKOWSKI 1948 | ESO 522-10, He 2- 378, Sa 2-320, VV' 379, Wray 16- 398 | 8.6 | -9.8 ± 13.3 | B: 16.9, V: 17.2 | |||||
PN G004.8-22.7 | 19 32 07 | -34 12 33 | He 2-436 | 4-22.1 | 19288-3419 | HENIZE 1964 | ESO 398-07, Sa 2-391, StWr 2-25 | < 10. | WC 4-5 | ||||||
PN G004.9-04.9 | 18 16 17 | -27 04 33 | M 1-44 | 4-04.2 | 18131-2705 | MINKOWSKI 1946 | ESO 522-11, He 2- 379, VV 165, VV' 380, Wray 16- 399 | 3.8 | -75.0 ± 11.0 | AG82 302, SS73 150 | K2 III | ||||
PN G005.0-03.9 | 18 12 23 | -26 32 55 | H 2-42 | 5-03.2 | HARO 1952 | ESO 522-02, VV' 365 | 11.8 | AG82 295 | B: 20.6 | ||||||
PN G005.1-03.0 | 18 09 13 | -26 02 26 | H 1-58 | 5-03.1 | 18061-2603 | HARO 1952 | ESO 521-34, Sa 2-303, VV' 354, Wray 17- 111 | 6.3 | B: 18.5, V: 17.4 | ||||||
PN G005.1-08.9 | 18 32 31 | -28 43 21 | Hf 2-2 | 5-08.1 | 18293-2845 | HOFFLEIT 1953 | ESO 457-16, He 2- 407, Sa 3-135, Wray 16- 414 | 18.6 | AG82 315 | B: 18.0 | |||||
PN G005.2-18.6 | 19 14 23 | -32 34 18 | StWr 2-21 | STOCK et al 1972 | ESO 397-07, Sa 2-383 | < 5. | |||||||||
PN G005.4-01.9 | 18 05 23 | -25 12 37 | PBOZ 34 | 18023-2513 | POTTASCH et al 1988 | 0. | < 1.6 | ||||||||
PN G005.5+02.7 | 17 48 08 | -22 46 47 | H 1-34 | 5+02.1 | 17451-2245 | HARO 1952 | ESO 520-28, VV' 253 | 0. | < 2. | ||||||
PN G005.5-02.5 | 18 07 53 | -25 24 02 | M 3-24 | 5-02.1 | 18048-2524 | MINKOWSKI 1948 | ESO 521-30, He 2- 350, Sa 2-300, VV'348, Wray 17- 110 | 10.2 | +128.0 ± 11.0 | ||||||
PN G005.5-04.0 | 18 13 40 | -26 08 43 | H 2-44 | 5-04.1 | 18105-2609 | HARO 1952 | ESO 522-07, Sa 3-124, VV' 371 | 6.6 | B: 18.2, V: 17.4 | ||||||
PN G005.6-04.7 | 18 16 54 | -26 23 24 | KFL 16 | KINMAN et al 1988 | 12.4 | +17.0 | |||||||||
PN G005.7-03.6 | 18 12 45 | -25 44 23 | KFL 13 | KINMAN et al 1988 | 14.2 | -71.0 | |||||||||
PN G005.7-05.3 | 18 19 25 | -26 35 19 | M 2-38 | 5-05.1 | 18163-2636 | MINKOWSKI 1947 | ARO 272, ESO 522-17, He 2- 388, Sa 2-328, VV 172, VV' 392, Wray 16- 406 | 9.3 | 7.4 | -72.3 ± 14.4 | B: 18.5, V: 17.4 | ||||
PN G005.8-06.1 | 18 22 54 | -26 49 17 | NGC 6620 | 5-06.1 | 18198-2650 | PICKERING 1880 | ARO 99, ESO 522-22, He 2- 394, Sa 2-332, StWr 2-4, VV 173, VV' 394, Wray 16-410 | 8.0 | 5. | +72.6 ± 0.4 | V: 19.6 | ||||
PN G005.9-02.6 | 18 09 12 | -25 04 35 | MaC 1-10 | 18061-2505 | MAC CONNELL 1978 | PM 1-213 | 10. | ||||||||
PN G006.0+02.8 | 17 48 37 | -22 16 49 | Th 4- 3 | 6+02.1 | 17456-2215 | THE 1964 | ARO 259, ESO 589-07, Sa 3- 78 | 0. | |||||||
PN G006.0+03.1 | 17 47 38 | -22 06 20 | M 1-28 | 6+03.2 | 17446-2205 | MINKOWSKI 1946 | ESO 589-06, He 2- 285, Sa 3- 76, VV 115, VV' 250 | 14.8 | +18.0 ± 5.0 | B: 21.6, V: 20.8 | |||||
PN G006.0-03.6 | 18 13 16 | -25 30 06 | M 2-31 | 6-03.3 | 18101-2530 | MINKOWSKI 1947 | ESO 522- 06, He 2- 368, Sa 2-313, StWr 2- 1, VV 158, VV' 369, Wray 16- 390 | 5.1 | 4. | +157.3 ± 10.1 | WC | ||||
PN G006.2+01.0 | 17 55 56 | -22 59 01 | HaTr 8 | HARTL et al 1983 | 12. | ||||||||||
PN G006.2-03.7 | 18 14 19 | -25 20 50 | KFL 15 | KINMAN et al 1988 | 8.5 | +123.0 | |||||||||
PN G006.3+03.3 | 17 47 34 | -21 47 25 | H 2-22 | 6+03.1 | 17445-2146 | HARO 1952 | ESO 589-05, Sa 3- 75, VV' 251 | 6.2 | |||||||
PN G006.4+02.0 | 17 52 41 | -22 21 57 | M 1-31 | 6+02.5 | 17496-2221 | MINKOWSKI 1946 | ESO 589-16, He 2- 299, Sa 2-260, Ve 59, VV 123, VV' 275 | 0. | 7.0 | +73.0 ± 5.0 | B: 19.0 | WC ? | |||
PN G006.4-04.6 | 18 18 14 | -25 38 11 | Pe 2-13 | 6-04.1 | 18150-2539 | PEREK 1960 | ESO 522-14, Sa 3-129, VV' 387 | 6.6 | B: 19.0, V: 17.3 | ||||||
PN G006.5-03.1 | 18 12 34 | -24 50 00 | H 1-61 | 6-03.1 | 18094-2450 | HARO 1952 | ESO 522-04, He 2- 364, VV' 364, Wray 16- 387 | 0. | +53.0 ± 5.0 | ||||||
PN G006.7-02.2 | 18 09 30 | -24 12 28 | M 1-41 | 6-02.1 | 18064-2413 | MINKOWSKI 1946 | He 2- 355, Ve 62, VV 152, VV' 355, Wray 17- 112 | 8.4 | -4.7 ± 2.6 | AG82 289 | (WN) ? | ||||
PN G006.8+02.0 | 17 53 37 | -21 58 41 | Pe 2-10 | 6+02.4 | PEREK 1960 | ESO 589-19, VV' 280 | 3.8 | ||||||||
PN G006.8+02.3 | 17 52 22 | -21 51 13 | Th 4- 7 | 6+02.3 | 17493-2150 | THE 1964 | ARO 263, ESO 589-15, Sa 2-257 | < 6. | 7.9 | ||||||
PN G006.8-03.4 | 18 14 28 | -24 43 33 | H 2-45 | 6-03.2 | 18114-2443 | HARO 1952 | ESO 522-08, Sa 2-315, VV' 374 | 4.6 | B: 18.2, V: 17.4 | ||||||
PN G006.8-08.6 | 18 34 55 | -27 06 23 | Al 1 | 18318-2708 | WRAY 1966 | ESO 523-02, Wray 15-1876 | 13. | AG82 321 | B: >18. | ||||||
PN G006.8-19.8 | 19 22 11 | -31 30 40 | Wray 16-423 | WRAY 1966 | ESO 459-17, Sa 2-389, StWr 2-18 | 0. | |||||||||
PN G007.0-06.0 | 18 24 57 | -25 41 54 | H 1-66 | 7-06.1 | 18218-2543 | HARO 1952 | AS 303, ESO 522-24, He 2- 397, MHa 366-101, Sa 2- 333, StWr 2-2, VV' 401 | 8.2 | 6.5 | +42.0 ± 25.0 | |||||
PN G007.0-06.8 | 18 27 59 | -26 06 41 | VY 2- 1 | 7-06.2 | 18248-2608 | VYSSOTSKY 1945 | ESO 522- 27, He 2- 400, Sa 2-336, StWr 2- 5, VV 181, VV' 405, Wray 15-1872 | < 7. | 3.7 | +115.0 ± 25.0 | B: 16.6 | WC ? | |||
PN G007.2+01.8 | 17 55 07 | -21 44 38 | Hb 6 | 7+01.1 | 17521-2144 | HUBBLE 1921 | ARO 96, ESO 589-20, He 2- 305, Sa 2-264, Ve 60, VV 128, VV' 285 | 5. | 6. | +9.2 ± 3.3 | 20.0 (O-III) | AG82 271, AN 265.1904, AS Sgr, HV 1146 | B: >16.4, V: >14.7 | ||
PN G007.8-03.7 | 18 17 16 | -23 58 51 | M 2-34 | 7-03.1 | MINKOWSKI 1947 | ESO 522-12, He 2- 382, Sa 3-127, VV 166, VV' 382, Wray 16- 402 | 8.4 | +70.0 ± 11.0 | WC 4-5 | ||||||
PN G007.8-04.4 | 18 20 09 | -24 15 06 | H 1-65 | 7-04.1 | 18170-2416 | HARO 1952 | ARO 273, AS 301, ESO 522-18, He 2- 389, MHa 304-145, VV' 393, Wray 16- 407 | 8. : | 2.5 | +161.0 ± 11.0 | B: 15.09, V: 14.67 | ||||
PN G008.0+03.9 | 17 49 15 | -20 00 34 | NGC 6445 | 8+03.1 | 17462-1959 | PICKERING 1882 | ARO 67, He 2- 290, Sa 2-248, ESO 589-09, VV 118, VV' 260 | 33. | > 34. | 2.5 | +16.2 ± 0.5 | 38.0 (O-III) | AG82 266, CSI -20 -17462, HD 161944 | B: 19.04, V: 19.00 | Contin. |
PN G008.1-04.7 | 18 22 01 | -24 10 40 | M 2-39 | 8-04.1 | 18189-2412 | MINKOWSKI 1947 | ESO 522-20, He 2- 391, Sa 2-329, VV 174, VV' 395, Wra y 15-1866 | 3.2 | +71.0 ± 5.0 | B: 16.2, V: 15.8 | |||||
PN G008.2-04.8 | 18 22 32 | -24 09 28 | M 2-42 | 8-04.2 | 18194-2410 | MINKOWSKI 1947 | ESO 522-21, He 2- 393, Sa 2-331, VV 177, VV' 398, Wray 16- 409 | 3.8 | +157.0 ± 25.0 | B: 18.2 | |||||
PN G008.3-01.1 | 18 08 25 | -22 16 53 | M 1-40 | 8-01.1 | 18054-2217 | MINKOWSKI 1946 | AS 278, ESO 590-02, He 2- 352, MHa 79- 25, Sa 2-302, VV 151, VV' 352 | 5. | 4.3 | -32.0 ± 11.0 | AG82 288 | B: 19.0, V: 18.3 | |||
PN G008.3-07.3 | 18 32 35 | -25 07 44 | NGC 6644 | 8-07.2 | 18295-2510 | PICKERING 1885 | ESO 522-23, He 2- 408, Sa 2-343, VV 188, VV' 417, Wray 16- 415 | 2.6 | 3. | +193.9 ± 1.3 | AG82 316, CD -25 13223, GCRV 10995, HD 170839 | B: 16.6, V: 15.6 | |||
PN G008.4-03.6 | 18 18 24 | -23 24 52 | H 1-64 | 8-03.1 | 18153-2326 | HARO 1952 | ESO 522-15, He 2-386, Sa 3-130, VV' 389, Wray 15-1857 | 7.6 | +84.0 ± 5.0 | ||||||
PN G008.6-02.6 | 18 14 51 | -22 43 55 | MaC 1-11 | MAC CONNELL 1978 | 0. | ||||||||||
PN G008.6-07.0 | 18 31 53 | -24 46 18 | He 2-406 | 8-07.1 | 18288-2448 | HENIZE 1964 | ARO 280, ESO 522-31, Sa 2-342, Wray 16- 413 | 3. : | |||||||
PN G009.0+04.1 | 17 50 28 | -19 03 12 | Th 4- 5 | 9+04.1 | 17475-1902 | THE 1964 | ESO 589-11, He 2- 293, Sa 2-252 | 6.4 | 7. | -18.0 ± 5.0 | |||||
PN G009.3+02.8 | 17 55 57 | -19 28 24 | Th 4- 9 | 9+02.1 | 17530-1929 | THE 1964 | ARO 266, ESO 589-21 | 0. | |||||||
PN G009.3+04.1 | 17 50 57 | -18 46 46 | Th 4- 6 | 9+04.2 | 17480-1846 | THE 1964 | ARO 262, ESO 589-12, Sa 2-254 | 0. | 5. | ||||||
PN G009.4-05.0 | 18 25 43 | -23 11 59 | NGC 6629 | 9-05.1 | 18226-2313 | HERSCHEL 1868 | ARO 30, ESO 522-26, He 2- 399, Sa 2-335, VV 179, VV' 403, Wray 15-1869 | 15.5 | 2.0 | +14.0 ± 3.0 | < 6.0 (O-III), 6.5 (N-II) | AG82 308, CD -23 14350, GCRV 10893, HD 169460 | B: 13.26, V: 12.93 | Of(H) | |
PN G009.4-09.8 | 18 44 43 | -25 21 34 | M 3-32 | 9-09.1 | 18416-2524 | MINKOWSKI 1948 | ESO 523-06, He 2- 420, Sa 2-362, VV' 445 | 6. | 7.5 | +46.0 ± 25.0 | B: 17.4, V: 17.1 | ||||
PN G009.6-10.6 | 18 48 12 | -25 28 49 | M 3-33 | 9-10.1 | 18451-2532 | MINKOWSKI 1948 | ESO 523-09, He 2- 423, Sa 2-367, VV' 452, Wray 16- 420 | 5. | 6. | +173.9 ± 10.1 | B: 15.7, V: 15.9 | ||||
PN G009.8-04.6 | 18 25 04 | -22 34 53 | H 1-67 | 9-04.1 | 18220-2236 | HARO 1952 | ESO 522-25, He 2- 398, Sa 2-334, VV' 402 | 5.6 | 6.8 | -13.0 ± 5.0 | |||||
PN G009.8-07.5 | 18 36 23 | -23 55 20 | GJJC 1 | GILLETT et al 1989 | 8.5 | -32.0 | U: 13.5, B: 14.8, V: 14.3 | ||||||||
PN G010.1+00.7 | 18 05 13 | -19 50 14 | NGC 6537 | 10+00.1 | 18021-1950 | PICKERING 1882 | ARO 52, ESO 590-01, He 2- 340, My 115, Sa 2-294, VV 147, VV' 339 | 10. | > 9. | 2.4 | -16.0 ± 3.0 | 18.0 (O-III) | AG82 284, CSI -19 -18023, GCRV 10524, HD 312582 | B: >19.8, V: >18.8 | |
PN G010.4+04.5 | 17 52 05 | -17 36 15 | M 2-17 | 10+04.1 | 17491-1735 | MINKOWSKI 1947 | ESO 589-14, He 2- 298, Sa 2-255, VV 122, VV' 274 | 6.4 | 8. | -21.0 ± 11.0 | |||||
PN G010.6+03.2 | 17 57 07 | -18 06 43 | Th 4-10 | 10+03.1 | 17541-1806 | THE 1964 | ESO 589-23, He 2- 311, Sa 3-99 | 0. | +29.3 ± 3.1 | B: 18.5, V: 18.3 | |||||
PN G010.7-06.4 | 18 33 55 | -22 38 40 | IC 4732 | 10-06.1 | 18308-2241 | FLEMING 1901 | ARO 71, ESO 523-01, He 2- 410, Sa 2-345, VV 191, VV' 424, Y-C 2- 24 | 4. | 1.2 | -145.4 ± 0.9 | AG82 320, BD -22 18309, CSI -22 -18309, HD 171131, NSV 11021 | B: >16.5, V: >16.2 | |||
PN G010.7-06.7 | 18 34 51 | -22 43 23 | Pe 1-13 | 10-06.2 | 18318-2245 | PEREK 1960 | ESO 523-03, Sa 2-348, VV' 427 | 7.6 | 5.6 | B: 18.0, V: 17.3 | |||||
PN G010.8-01.8 | 18 16 17 | -20 26 59 | NGC 6578 | 10-01.1 | 18132-2028 | PICKERING 1882 | ARO 70, ESO 590-12, He 2- 381, Sa 2-322, VV 163, VV' 376 | 8.5 | 2.0 | +4.5 ± 1.8 | AG82 303 | B: 16.30, V: 15.82 | WC early | ||
PN G011.0+05.8 | 17 48 20 | -16 28 44 | NGC 6439 | 11+05.1 | 17454-1627 | PICKERING 1882 | ARO 95, He 2- 287, Sa 2-245, VV 117, VV' 256, Y-C 2- 21 | 5. | 4. | 1.3 | -93.8 ± 1.8 | 24.0 (O-III) | AG82 265, CSI -16 -17453, HD 161801 | B: 20.2 | |
PN G011.0+06.2 | 17 46 54 | -16 17 24 | M 2-15 | 11+06.1 | 17440-1616 | MINKOWSKI 1947 | He 2- 284, Sa 2-242, VV 114, VV' 249 | 5.8 | 7.5 | +3.7 ± 10.1 | B: 17.8, V: 18.2 | ||||
PN G011.0-05.1 | 18 29 11 | -21 46 53 | M 1-47 | 11-05.1 | 18261-2148 | MINKOWSKI 1946 | ESO 591-02, He 2- 403, Sa 2-338, VV 184, VV' 409 | 4.6 | 5.5 | -72.2 ± 10.1 | B: 15.4, V: 15.3 | ||||
PN G011.3+02.8 | 18 00 09 | -17 40 30 | Th 4-11 | 11+02.1 | 17572-1740 | THE 1964 | ARO 267, ESO 589-25, He 2- 322 | < 5. | |||||||
PN G011.3-09.4 | 18 46 34 | -23 26 50 | H 2-48 | 11-09.1 | 18435-2330 | HARO 1952 | AS 957, ESO 523-07, He 2- 422, MHa 152- 1, My 121, SaSt 2-23, VV' 449, Wray 16-419, Y-C 2- 30 | 2. | 1.7 | -21.0 | 5.0 (O-III), 2.5 (N-II) | B: 13.78, V: 13.41 | |||
PN G011.7-00.0 | 18 11 48 | -18 46 03 | M 1-43 | 11-00.1 | MINKOWSKI 1946 | ESO 590-05, He 2- 363, VV 156, Sa 3-122, VV' 361 | 5.2 | B: 17.2, V: 16.0 | |||||||
PN G011.7-00.6 | 18 13 45 | -19 04 19 | NGC 6567 | 11-00.2 | 18108-1905 | PICKERING 1882 | ARO 69, ESO 590-08, He 2-369, Sa 2-314, VV 160, VV' 372 | 7.6 | 1.6 | +119.3 ± 0.7 | 18.4 (O-III), 36. (N-II) | AG82 297, BD -19 18107, CSI -19 -18107, HD 166935 | B: 14.42, V: 14.36 | WC | |
PN G011.7-06.6 | 18 36 34 | -21 48 57 | M 1-55 | 11-06.1 | 18335-2151 | MINKOWSKI 1946 | ESO 591-10, He 2- 414, SaSt 2-22, VV 195, VV' 431 | 0. | -22.0 ± 5.0 | B: 13.94, V: 13.90 | O ? | ||||
PN G011.9+04.2 | 17 56 19 | -16 29 01 | M 1-32 | 11+04.1 | 17534-1628 | MINKOWSKI 1946 | He 2- 309, Sa 2-268, VV 130, VV' 292 | 7.6 | 9. | -72.8 ± 14.0 | AG82 274 | B: 18.3, V: 17.0 | WC 4-6 | ||
PN G012.5-09.8 | 18 50 26 | -22 34 22 | M 1-62 | 12-09.1 | 18474-2237 | MINKOWSKI 1946 | ESO 523-10, He 2- 424, Sa 2-369, VV 207, VV' 457 | 3.6 | 1.5 | +34.0 ± 25.0 | B: 16.9, V: 17.4 | WC ? | |||
PN G012.6-02.7 | 18 23 08 | -19 17 06 | M 1-45 | 12-02.1 | 18201-1918 | MINKOWSKI 1946 | ARO 276, ESO 590-18, He 2- 395, VV 178, VV' 399 | 0. | 2.5 | +126.0 ± 11.0 | B: 18.0, V: 16.8 | ||||
PN G013.0-04.3 | 18 29 59 | -19 40 38 | Pe 2-14 | 13-04.1 | 18271-1942 | PEREK 1960 | ESO 591-04, Sa 2-340, VV' 412 | 5. | |||||||
PN G013.4-03.9 | 18 29 30 | -19 05 45 | M 1-48 | 13-03.1 | 18265-1908 | MINKOWSKI 1946 | ESO 591-03, He 2- 404, Sa 2-339, VV 185, VV' 411 | 4.8 | 5.5 | +140.0 ± 25.0 | |||||
PN G013.7-10.6 | 18 55 31 | -21 49 39 | Y-C 2-32 | 18525-2153 | CESCO et al 1973 | ESO 592-06, Sa 2-376 | 15. : | B: 16.6, V: 16.7 | |||||||
PN G013.8-02.8 | 18 26 03 | -18 12 06 | SaWe 3 | SAURER et al 1987 | 110. | 12.5 (O-III) | |||||||||
PN G013.8-07.9 | 18 45 35 | -20 35 00 | PC 21 | 13-07.1 | PEIMBERT et al 1961 | ESO 591-16, Sa 2-364, Y-C 2-28 | 13.2 | B: 18.4 | |||||||
PN G014.0-05.5 | 18 36 32 | -19 19 27 | V-V 3-5 | 18335-1922 | VORONCOV-VEL'JAMINOV et al 1972 | ESO 591-09, He 3-1716, Sa 1- 7, Sa 2-351, V-V Anon.2 | 0. | B: 13.66, V: 13.27 | A | ||||||
PN G014.2-07.3 | 18 44 02 | -19 54 55 | M 3-31 | 14-07.1 | 18410-1958 | MINKOWSKI 1948 | ESO 591-15, He 2- 419, Sa 2-361, VV' 444 | 7. : | 0.9 | -88.6 ± 4.7 | B: 17.7, V: 17.4 | ||||
PN G014.3-05.5 | 18 37 11 | -19 02 22 | V-V 3-6 | 18342-1904 | VORONCOV-VEL'JAMINOV et al 1972 | ESO 591-11, Sa 2-352, V-V Anon. 3, Y-C 2-25 | 0. | 1. | |||||||
PN G014.6-04.3 | 18 33 21 | -18 16 30 | M 1-50 | 14-04.1 | 18304-1818 | MINKOWSKI 1946 | ESO 591-07, He 2- 409, Sa 2-344, VV 189, VV' 421, Y-C 2- 23 | 5.6 | +27.1 ± 10.1 | AG82 317 | Contin.? | ||||
PN G014.7-11.8 | 19 02 16 | -21 26 51 | SaWe 4 | SAURER et al 1987 | 85. | ||||||||||
PN G014.8-25.6 | 19 58 13 | -26 28 15 | HDW 12 | HARTL et al 1983 | HaWe 14 | 46. | AG82 391 | B: 17.7 | |||||||
PN G014.9-03.1 | 18 29 11 | -17 27 13 | SaSt 3-166 | SANDULEAK et al 1973 | 13. : | ||||||||||
PN G015.4-04.5 | 18 35 48 | -17 36 08 | M 1-53 | 15-04.1 | 18328-1738 | MINKOWSKI 1946 | ESO 591-08, He 2- 412, Sa 2-349, VV 193, VV' 428 | 6. | +63.0 ± 25.0 | 13.0 (O-III) | B: 15.52, V: 14.30 | ||||
PN G015.6-03.0 | 18 30 11 | -16 45 27 | A 44 | 15-03.1 | ABELL 1955 | A55 32, ARO 278, VV' 413 | 53. | +44.0 ± 6.0 | 6.0 (O-III) | ||||||
PN G016.0-04.3 | 18 36 08 | -16 59 59 | M 1-54 | 16-04.1 | 18332-1702 | MINKOWSKI 1946 | He 2- 413, Sa 2-350, VV 194, VV' 430 | 13. | -40.6 ± 10.1 | ||||||
PN G016.1-04.7 | 18 37 46 | -17 05 47 | M 1-56 | 16-04.2 | 18348-1708 | MINKOWSKI 1946 | He 2- 415, Sa 2-353, VV 196, VV' 432 | < 10. | 1.4 | +88.0 ± 25.0 | B: 16.7, V: 16.2 | ||||
PN G017.3-21.9 | 19 46 34 | -23 08 12 | A 65 | 17-21.1 | 19435-2315 | ABELL 1964 | ARO 26, ESO 526-03, Sh 2- 52, VV' 513 | 100. | +13.0 ± 4.0 | 11.0 (O-III) | AG82 384, CSI -23 -19436, UBV 16806 | U: 15.01, B: 15.99, V: 15.90 | Op k | ||
PN G017.6-10.2 | 19 01 01 | -18 12 15 | A 51 | 17-10.1 | 18581-1816 | ABELL 1955 | A55 38, ARO 300, VV' 471 | 67. | +23.0 ± 10.0 | 42.0 (O-III) | AG82 337, CSI -18 -18581, UBV 16133 | U: 14.26, B: 15.30, V: 15.42 | sd O8k, OH | ||
PN G019.4-13.6 | 19 17 05 | -18 01 34 | DeHt 3 | DENGEL et al 1980 | ESO 593-09, DHW 1-1 | 32. | |||||||||
PN G019.4-19.6 | 19 40 32 | -20 27 00 | K 2- 7 | 19-19.1 | KOHOUTEK 1962 | ESO 594-10 | 140. | AG82 377 | B: 19.3 | ||||||
PN G019.8-23.7 | 19 57 32 | -21 36 37 | A 66 | 19-23.1 | 19545-2144 | ABELL 1955 | A55 53, ARO 339, ESO 595-04, VV' 519 | 267. | AG82 389, CSI -21 -19546, UBV 16998 | U: 16.84, B: 17.71, V: 17.39 | |||||
PN G025.0-11.6 | 19 19 17 | -12 14 52 | A 60 | 25-11.1 | ABELL 1955 | A55 47, ARO 314, VV' 493 | 74. | AG82 364 | B: 18.5 | ||||||
PN G025.8-17.9 | 19 43 58 | -14 09 07 | NGC 6818 | 25-17.1 | 19411-1416 | HERSCHEL 1787 | ARO 12, Sa 2-392, VV 241, VV' 511 | 20. | 2.2 | -13.0 ± 3.0 | 27.6 (O-III), 31. (N-II) | AG82 381 | B: 16.90 | WNb ? | |
PN G355.1-06.9 | 18 02 31 | -36 38 51 | M 3-21 | 355-06.1 | 17591-3639 | MINKOWSKI 1948 | ESO 394-21, He 2- 328, Sa 2-284, VV' 319, Wray 16- 352 | < 5. | -68.6 ± 3.8 | AG82 280, CSI -36-17592 0, GCRV 10455, HV7117, V567 Sgr | B: 16.2, V: 15.3 | ||||
PN G356.3-06.2 | 18 02 32 | -35 13 08 | M 3-49 | 356-06.1 | MINKOWSKI 1948 | ESO 394-22, He 2- 329, Sa 3-112, VV' 318, Wray 16- 353 | 9.8 | -47.0 ± 5.0 | |||||||
PN G356.6-07.8 | 18 09 49 | -35 44 12 | H 1-57 | 356-07.2 | HARO 1952 | ESO 394-31, He 2- 353, Sa 3-121, VV' 353, Wray 17- 113 | 12.6 | ||||||||
PN G356.7-06.4 | 18 04 29 | -34 58 00 | H 1-51 | 356-06.2 | HARO 1952 | ESO 394-26, Sa 3-116, VV' 331, Wray 16- 362 | 13.2 | ||||||||
PN G356.9-05.8 | 18 02 03 | -34 27 47 | M 2-24 | 356-05.2 | 17587-3427 | MINKOWSKI 1947 | ESO 394-20, He 2- 327, Sa 2-282, VV 137, VV' 317, Wray 16- 351 | 6.8 | +173.0 ± 11.0 | ||||||
PN G357.1-06.1 | 18 04 05 | -34 28 31 | M 3-50 | 357-06.1 | MINKOWSKI 1948 | ESO 394-25, Sa 2-290, VV' 327 | 4. | +24.0 ± 11.0 | |||||||
PN G358.0-05.1 | 18 01 43 | -33 15 18 | Pe 1-11 | 358-05.1 | 17584-3315 | MINKOWSKI 1948 | ESO 394-19, Sa 2-280, VV' 315, Wray 16- 349 | 8.8 | |||||||
PN G358.5-07.3 | 18 12 03 | -33 52 01 | NGC 6563 | 358-07.1 | 18087-3352 | HERSCHEL 1837 | ARO 503, CD -33 12935, ESO 394-33, GCRV 10633, He 2- 361, HD 166469, Sa 2- 308, StWr 2- 22, VV 154, VV' 359, Wray 16-383 | 47.5 | 0.8 | -29.5 ± 5.1 | 11.0 (O-III) | AG82 293 | B: 17.33 | ||
PN G358.6-05.5 | 18 04 56 | -32 54 04 | M 3-51 | 358-05.4 | MINKOWSKI 1948 | ESO 394-27, He 2- 337, Sa 3- 118, VV' 334, Wray 16- 365 | 9.2 | +34.0 ± 11.0 | |||||||
PN G358.7-05.2 | 18 03 54 | -32 41 38 | H 1-50 | 358-05.3 | 18006-3241 | HARO 1952 | ESO 394-24, He 2- 334, Sa 2-288, VV' 325, Wray 16- 359 | < 10. | 1.4 | +28.0 ± 25.0 | V: 17.1 | ||||
PN G359.0-04.8 | 18 02 47 | -32 09 31 | M 2-25 | 359-04.3 | 17594-3209 | MINKOWSKI 1947 | ESO 456-40, He 2- 330, Sa 2-285, VV 138, VV' 321, Wray 16- 354 | 14. | +20.0 ± 11.0 | ||||||
PN G359.2-33.5 | 20 19 28 | -41 31 30 | CRBB 1 | MAC CARTHY 1991 | He 3-1863 | 8. | CD-41 13967 | U: 9.60, B: 10.56 | O(H) | ||||||
PN G359.3-00.9 | 17 47 57 | -29 59 53 | Hb 5 | 359-00.1 | 17447-2958 | HUBBLE 1921 | ARO 389, Bl E, ESO 455-42, He 2- 286, VV 116, VV' 252, Wray 16- 310 | 15. | > 13. | 2.0 | -28.0 ± 5.0 | AG82 264, CD -29 13998, HD 316340 | B: 18.6 | ||
PN G359.6-04.8 | 18 04 07 | -31 39 13 | H 2-36 | 359-04.4 | HARO 1952 | ESO 456-45, Sa 3-114, VV' 329, Wray 16- 361 | 9.9 | ||||||||
PN G359.7-04.4 | 18 02 53 | -31 23 57 | KFL 3 | KINMAN et al 1988 | 13.5 | +200.0 | |||||||||
PN G359.8-07.2 | 18 14 50 | -32 37 09 | M 2-32 | 359-07.1 | 18115-3237 | MINKOWSKI 1957 | ESO 394-35, He 2- 371, Sa 2-316, StWr 2-19, VV 161, VV' 373, Wray 16- 393 | < 10. | -49.4 ± 10.1 | B: 15.5, V: 15.7 | |||||
PN G359.9-04.5 | 18 03 52 | -31 17 45 | M 2-27 | 359-04.2 | 18006-3117 | MINKOWSKI 1947 | ESO 456-44, He 2- 335, Sa 2-289, VV 140, VV' 326, Wray 16- 360 | 4.8 | 2.5 | +170.4 ± 12.2 | |||||
PN G359.9-05.4 | 18 07 19 | -31 42 54 | KFL 9 | KINMAN et al 1988 | 11.8 | -19.0 |
ID | Name | RA | Dec | RSun | RGC | Fe/H | wt | EB-V | VHB | (m-M)V | Vt | MV,t | U-B | B-V | V-R | V-I | spt | ellip | vr | vLSR | sigv | c | rc | rh | μV | ρ0 | lg(tc) | lg(th) |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Terzan 5 | Terzan 11 | 17 48 04.80 | -24 46 45 | 6.9 | 1.2 | -0.23 | 3 | 2.28 | 22.04 | 21.27 | 13.85 | -7.42 | 2.13 | 2.77 | -93.0 ± 2.0 | -83.5 | 1.62 | 0.16 | 0.72 | 21.08 | 5.14 | 7.57 | 8.53 | |||||
NGC 6440 | 17 48 52.70 | -20 21 36.9 | 8.5 | 1.3 | -0.36 | 6 | 1.07 | 18.70 | 17.95 | 9.20 | -8.75 | 1.47 | 1.97 | 1.24 | 2.51 | G4 | 0.01 | -76.6 ± 2.7 | -65.9 | 1.62 | 0.14 | 0.48 | 17.06 | 5.24 | 7.60 | 8.62 | ||
UKS 1 | 17 54 27.2 | -24 08 43 | 7.8 | 0.7 | -0.64 | 2 | 3.14 | 24.90 | 24.20 | 17.29 | -6.91 | 57.0 ± 6.0 | 66.7 | 2.10 | 0.15 | 25.52 | 4.41 | 7.26 | 0.00 | |||||||||
Terzan 9 | 18 01 38.8 | -26 50 23 | 7.1 | 1.1 | -1.05 | 2 | 1.76 | 20.35 | 19.71 | 16.00 | -3.71 | 59.0 ± 10.0 | 68.1 | 2.50 c | 0.03 | 0.78 | 23.21 | 4.42 | 4.99 | 8.00 | ||||||||
Djorg 2 | ESO456-SC38 | 18 01 49.1 | -27 49 33 | 6.3 | 1.8 | -0.65 | 1 | 0.94 | 17.60 | 16.90 | 9.90 | -7.00 | 1.50 | 0.33 | 1.05 | 19.50 | 3.85 | 7.73 | 0.00 | |||||||||
NGC 6522 | 18 03 34.02 | -30 02 02.3 | 7.7 | 0.6 | -1.34 | 4 | 0.48 | 16.52 | 15.92 | 8.27 | -7.65 | 0.65 | 1.21 | 0.76 | 1.51 | F7/8 | 0.06 | -21.1 ± 3.4 | -12.9 | 6.7 ± 0.7 | 2.50 c | 0.05 | 1.00 | 15.75 | 5.48 | 6.38 | 8.86 | |
Terzan 10 | 18 03 36.4 | -26 04 21 | 5.8 | 2.3 | -1.00 | 1 | 2.40 | 21.90 | 21.25 | 14.90 | -6.35 | 0.75 | 0.90 | 1.55 | 21.28 | 4.64 | 9.34 | 8.74 | ||||||||||
NGC 6528 | 18 04 49.64 | -30 03 22.6 | 7.9 | 0.6 | -0.11 | 7 | 0.54 | 16.95 | 16.17 | 9.60 | -6.57 | 1.09 | 1.53 | 0.90 | 1.74 | G3 | 0.11 | 206.6 ± 1.4 | 214.9 | 1.50 | 0.13 | 0.38 | 16.73 | 4.77 | 7.28 | 8.06 | ||
NGC 6540 | Djorg 3 | 18 06 08.6 | -27 45 55 | 5.3 | 2.8 | -1.35 | 2 | 0.66 | 16.25 | 15.65 | 9.30 | -6.35 | -17.7 ± 1.4 | -8.8 | 2.50 | 0.03 | 16.40 | 5.85 | 5.40 | 0.00 | ||||||||
NGC 6544 | 18 07 20.58 | -24 59 50.4 | 3.0 | 5.1 | -1.40 | 4 | 0.76 | 15.30 | 14.71 | 7.77 | -6.94 | 0.73 | 1.46 | 0.98 | 1.92 | F9 | 0.22 | -27.3 ± 3.9 | -17.7 | 1.63 c: | 0.05 | 1.21 | 16.31 | 6.06 | 5.35 | 8.24 | ||
2MS-GC01 | 2MASS-GC01 | 18 08 21.81 | -19 49 47 | 3.6 | 4.5 | 0 | 6.80 | 34.50 | 33.85 | 27.74 | -6.11 | 0.85 | 0.85 | 1.65 | 8.43 | |||||||||||||
NGC 6553 | 18 09 17.60 | -25 54 31.3 | 6.0 | 2.2 | -0.18 | 6 | 0.63 | 16.60 | 15.83 | 8.06 | -7.77 | 1.34 | 1.73 | 1.01 | 2.13 | G4 | 0.17 | -3.2 ± 1.5 | 6.1 | 1.16 | 0.53 | 1.03 | 18.17 | 3.84 | 8.24 | 8.72 | ||
2MS-GC02 | 2MASS-GC02 | 18 09 36.50 | -20 46 44 | 4.9 | 3.2 | -1.08 | 1 | 5.16 | 30.10 | 29.46 | 24.60 | -4.86 | -238.0 ± 36.0 | -227.4 | 0.95 | 0.55 | 0.55 | 7.72 | ||||||||||
NGC 6558 | 18 10 17.60 | -31 45 50.0 | 7.4 | 1.0 | -1.32 | 5 | 0.44 | 16.30 | 15.70 | 9.26 | -6.44 | 0.58 | 1.11 | 0.71 | 1.46 | F7 | -197.2 ± 1.5 | -189.4 | 3.1 ± 0.9 | 2.50 c | 0.03 | 2.15 | 16.48 | 5.35 | 5.71 | 9.12 | ||
Terzan 12 | 18 12 15.8 | -22 44 31 | 4.8 | 3.4 | -0.50 | 1 | 2.06 | 20.50 | 19.77 | 15.63 | -4.14 | 94.1 ± 1.5 | 104.2 | 0.57 | 0.83 | 0.75 | 23.75 | 3.40 | 8.46 | 7.78 | ||||||||
NGC 6569 | 18 13 38.80 | -31 49 36.8 | 10.9 | 3.1 | -0.76 | 4 | 0.53 | 17.52 | 16.83 | 8.55 | -8.28 | 0.74 | 1.34 | 0.83 | 1.69 | G1 | 0.00 | -28.1 ± 5.6 | -20.3 | 1.31 | 0.35 | 0.80 | 18.15 | 3.63 | 8.38 | 9.05 | ||
BH 261 | AL 3 | 18 14 06.6 | -28 38 06 | 6.5 | 1.7 | -1.30 | 1 | 0.36 | 15.80 | 15.19 | 11.00 | -4.19 | 0.03 | 1.00 | 0.40 | 0.55 | 7.80 | |||||||||||
GLIMPSE02 | 18 18 30.5 | -16 58 38 | 5.5 | 3.0 | -0.33 | 1 | 7.85 | 38.80 | 38.05 | 1.33 | 0.70 | |||||||||||||||||
NGC 6624 | 18 23 40.51 | -30 21 39.7 | 7.9 | 1.2 | -0.44 | 4 | 0.28 | 16.09 | 15.36 | 7.87 | -7.49 | 0.60 | 1.11 | 0.67 | 1.42 | G4/5 | 0.06 | 53.9 ± 0.6 | 62.1 | 5.4 ± 0.5 | 2.50 c | 0.06 | 0.82 | 15.32 | 5.30 | 6.61 | 8.71 | |
NGC 6626 | M 28 | 18 24 32.81 | -24 52 11.2 | 5.5 | 2.7 | -1.32 | 2 | 0.40 | 15.55 | 14.95 | 6.79 | -8.16 | 0.46 | 1.08 | 0.69 | 1.41 | F8 | 0.16 | 17.0 ± 1.0 | 26.6 | 8.6 ± 1.3 | 1.67 | 0.24 | 1.97 | 15.77 | 4.86 | 7.62 | 9.17 |
NGC 6638 | 18 30 56.10 | -25 29 50.9 | 9.4 | 2.2 | -0.95 | 4 | 0.41 | 16.80 | 16.14 | 9.02 | -7.12 | 0.56 | 1.15 | 0.72 | 1.50 | G0 | 0.01 | 18.1 ± 3.9 | 27.5 | 1.33 | 0.22 | 0.51 | 17.30 | 4.09 | 7.83 | 8.46 | ||
NGC 6637 | M 69 | 18 31 23.10 | -32 20 53.1 | 8.8 | 1.7 | -0.64 | 4 | 0.18 | 15.98 | 15.28 | 7.64 | -7.64 | 0.48 | 1.01 | 0.62 | 1.28 | G2/3 | 0.01 | 39.9 ± 2.8 | 47.5 | 1.38 | 0.33 | 0.84 | 16.82 | 3.84 | 8.15 | 8.82 | |
NGC 6642 | 18 31 54.10 | -23 28 30.7 | 8.1 | 1.7 | -1.26 | 5 | 0.40 | 16.40 | 15.79 | 9.13 | -6.66 | 0.57 | 1.11 | 0.72 | 1.45 | F8 | 0.03 | -57.2 ± 5.4 | -47.3 | 1.99 c: | 0.10 | 0.73 | 16.82 | 4.64 | 6.95 | 8.52 | ||
NGC 6652 | 18 35 45.63 | -32 59 26.6 | 10.0 | 2.7 | -0.81 | 4 | 0.09 | 15.96 | 15.28 | 8.62 | -6.66 | 0.37 | 0.94 | 0.52 | 1.08 | G3 | 0.20 | -111.7 ± 5.8 | -104.3 | 1.80 | 0.10 | 0.48 | 16.10 | 4.48 | 7.05 | 8.39 | ||
NGC 6656 | M 22 | 18 36 23.94 | -23 54 17.1 | 3.2 | 4.9 | -1.70 | 8 | 0.34 | 14.15 | 13.60 | 5.10 | -8.50 | 0.28 | 0.98 | 0.68 | 1.42 | F5 | 0.14 | -146.3 ± 0.2 | -136.6 | 7.8 ± 0.3 | 1.38 | 1.33 | 3.36 | 17.42 | 3.63 | 8.53 | 9.23 |
Pal 8 | 18 41 29.9 | -19 49 33 | 12.8 | 5.5 | -0.37 | 3 | 0.32 | 17.27 | 16.53 | 11.02 | -5.51 | 0.72 | 1.22 | -43.0 ± 15.0 | -32.3 | 1.53 | 0.56 | 0.58 | 20.00 | 2.34 | 8.65 | 8.47 | ||||||
NGC 6681 | M 70 | 18 43 12.76 | -32 17 31.6 | 9.0 | 2.2 | -1.62 | 3 | 0.07 | 15.55 | 14.99 | 7.87 | -7.12 | 0.12 | 0.72 | 0.47 | 0.99 | F5 | 0.01 | 220.3 ± 0.9 | 227.8 | 5.2 ± 0.5 | 2.50 c | 0.03 | 0.71 | 14.25 | 5.82 | 5.82 | 8.65 |
NGC 6715 | M 54 | 18 55 03.33 | -30 28 47.5 | 26.5 | 18.9 | -1.49 | 7 | 0.15 | 18.16 | 17.58 | 7.60 | -9.98 | 0.24 | 0.85 | 0.53 | 1.10 | F7/8 | 0.06 | 141.3 ± 0.3 | 149.2 | 10.5 ± 0.3 | 2.04 | 0.09 | 0.82 | 14.78 | 4.69 | 8.24 | 9.93 |
NGC 6717 | Pal 9 | 18 55 06.04 | -22 42 05.3 | 7.1 | 2.4 | -1.26 | 3 | 0.22 | 15.55 | 14.94 | 9.28 | -5.66 | 0.35 | 1.00 | 0.65 | 1.37 | F6 | 0.01 | 22.8 ± 3.4 | 32.7 | 2.07 | 0.08 | 0.68 | 16.77 | 4.58 | 6.52 | 8.22 | |
NGC 6723 | 18 59 33.15 | -36 37 56.1 | 8.7 | 2.6 | -1.10 | 3 | 0.05 | 15.48 | 14.84 | 7.01 | -7.83 | 0.21 | 0.75 | 0.50 | 1.05 | F9 | 0.00 | -94.5 ± 3.6 | -88.3 | 1.11 c: | 0.83 | 1.53 | 18.13 | 2.79 | 8.79 | 9.24 | ||
Terzan 7 | 19 17 43.92 | -34 39 27.8 | 22.8 | 15.6 | -0.32 | 6 | 0.07 | 17.76 | 17.01 | 12.00 | -5.01 | 166.0 ± 4.0 | 172.5 | 0.93 | 0.49 | 0.77 | 20.66 | 1.63 | 8.89 | 8.96 | ||||||||
Arp 2 | 19 28 44.11 | -30 21 20.3 | 28.6 | 21.4 | -1.75 | 5 | 0.10 | 18.13 | 17.59 | 12.30 | -5.29 | 0.86 | 115.0 ± 10.0 | 122.4 | 0.88 | 1.19 | 1.77 | 24.26 | -0.25 | 9.39 | 9.70 | |||||||
NGC 6809 | M 55 | 19 39 59.71 | -30 57 53.1 | 5.4 | 3.9 | -1.94 | 4 | 0.08 | 14.40 | 13.89 | 6.32 | -7.57 | 0.11 | 0.72 | 0.48 | 1.00 | F4 | 0.02 | 174.7 ± 0.3 | 181.8 | 4.0 ± 0.3 | 0.93 | 1.80 | 2.83 | 19.36 | 2.22 | 8.90 | 9.29 |
Terzan 8 | 19 41 44.41 | -33 59 58.1 | 26.3 | 19.4 | -2.16 | 2 | 0.12 | 17.95 | 17.47 | 12.40 | -5.07 | 130.0 ± 8.0 | 136.2 | 0.60 | 1.00 | 0.95 | 22.82 | 0.53 | 9.46 | 9.21 | ||||||||
NGC 6864 | M 75 | 20 06 04.69 | -21 55 16.2 | 20.9 | 14.7 | -1.29 | 3 | 0.16 | 17.70 | 17.09 | 8.52 | -8.57 | 0.28 | 0.87 | 0.55 | 1.16 | F9 | 0.07 | -189.3 ± 3.6 | -180.8 | 10.3 ± 1.5 | 1.80 | 0.09 | 0.46 | 15.52 | 4.51 | 7.89 | 9.15 |