Constellation Scorpius (Scorpion)

Scorpius
Scorpius: IAU Constellation Map [150]

Properties

Despite an area of 497 square degrees, Scorpius is a large, bright and impressive constellation and is one of the most beautiful in the sky. It is partially located in the band of the Milky Way, near its center, west of Sagittarius. The outlines of this constellation are very reminiscent of the shape of this animal: the threateningly outstretched claws lie in the constellation Libra; the striking star formation around Antares, the heart of the scorpion, represents the breastplate; even the tail with the poison sting, raised to attack, is indicated by a star bow. The center of the constellation culminates around midnight on June 3rd. [9, 15]

Stars with Proper Names:

  • α Sco: Antares, Cor Scorpii, Kalb Al Akrab, Vespertilio
  • β1 Sco: Graffias, Grafias, Grassias, Acrab, Akrab, Elacrab
  • δ Sco: Dschubba, Iclarkrau
  • θ Sco: Sargas
  • λ Sco: Shaula
  • ν Sco: Jabbah
  • σ Sco: Alniyat, Al Niyat
  • υ Sco: Lesath, Lesuth
Data for constellation Scorpius [150]
IAU NameScorpius
IAU GenitiveScorpii
IAU Abbr.Sco
English NameScorpion
Season (47° N)April … August
Right Ascension15h 47m 15s … 17h 59m 14s
Declination-45° 46' 01" … -08° 17' 45"
Area497 deg2
Neighbours (N↻)Oph, Lib, Lup, Nor, Ara, CrA, Sgr

Deep-Sky Object Descriptions

Ophiuchus Molecular Cloud
Ophiuchus Molecular Cloud: Star forming region with open cluster Collinder 302 with Ophiuchus molecular cloud (Antares Nebula vdB 107, nebula IC 4603, ρ Ophiuchi nebula IC 4604, nebula IC 4605, Sharpless 2-9, many dark clouds), plus globular clusters M 4 and NGC 6144. North is left; Canon EOS 20Da, zoom lens 131 mm f:5.6 ; 145 min @ ISO 1600; Astrofarm Tivoli, Namibia, 1345 m ü. M.; © 5. 6. 2011 Eduard von Bergen, Hansjörg Wälchli

Mythology and History

According to rock carvings in the Caucasus region, the constellation of Scorpio was already in the 3rd millennium BC. Known, but the scorpion also appears in the Orion legend:

Orion was a mighty hunter who knew how to captivate even goddesses in love because of his beautiful figure. Jealousy and resentment were the result, which finally cost the Orion his life. In another version of death, the scorpion plays a role. Gäa, the earth goddess sent Orion a poisonous scorpion because he bragged that there was no animal he could not kill. Orion is said to have died of a scorpion sting, or the Sagittarius came to him just in time Help? As a punishment, the scorpion was moved to a place in the sky that is almost exactly opposite the Orion, so that Orion rises when the scorpion goes down. [20]

Scorpius + Libra
Scorpius + Libra: Complete Scorpius constellation before Caesar, when Scorpio still had claws [265]

The ancient Greeks counted the area, where today the constellation Libra is located, still to Scorpius and saw here the claws of the scorpion. This is the origin of the Arabic names of the stars. During Julius Caesar's lifetime, the Romans separated into this area and formed the independent constellation and zodiac sign Libra.

Indians from central Brazil see the Scorpion as a carrying net for children. Indians from the Rio Negro river basin in northern Brazil see the scorpion as a big snake with a wide open mouth and a twisted body. The bright Antares is the snake's prey to be strangled down. At the end of the tail lies the egg of the snake. [20] The Indians of the North American tribe of the Navajo interpreted the four stars, which form the stache of the scorpion, as the footprint of a running hare. The first appearance of this constellation at dawn heralded the approach of spring. [61, 107]

Constellation Scorpio
Constellation Scorpio: Illustration from «Uranometria» by Johann Bayer, copper engraving by Alexander Mair, 1603 [28]

Catalogs

Yale Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991) [154]
HR B F DM HD SAO FK5 IR M* ADS VarID RA Dec vMag spType dMag Sep ["] Remarks
HR 58851CD-2511131141637183854 15 50 58.7-25 45 054.64 B3V G:Sco OB2 assoc.; probable member of Sco-Cen cluster; upper Sco region; embedded in reflection nebulosity; member of,G:Pleiades group.,RV:Rapidly rotating star which might become Be star.
HR 59042CD-24123521421141838969823 15 53 36.7-25 19 384.59 B2.5Vn 2.52.3D:CPM. Combined mag., color.,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco region; embedded in reflection nebulosity.,RV:Rapidly rotating star which may become Be star.
HR 5906CD-2412354142165183900D 15 53 53.8-24 31 595.39 B6IVn D:Suspected occultation double.,G:Sco OB2; Sco-Cen assoc.; doubtful member of the Sco-Cen cluster; upper Sco region.
HR 5907CD-2312569142184183901 7314 15 53 55.8-23 58 415.42 B2.5Vne G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster; upper Sco region.,VAR:Amp. 0.03V on time scale 2 hrs. suspected.
HR 5910CD-2611096142250183907 15 54 30.0-27 20 196.14 B6Vp G:Sco OB2.,RV:Determinations of vsini range from 29 to 196k/s.
HR 59123CD-2412365142301183914 V927 Sco15 54 39.5-25 14 375.87 B8IIIp G:Sco OB2.,S:Helium-weak star.,VAR:1.45937d. Magnetic field variable 1.45955d (Landstreet et al. 1979, MNRAS, 188, 609).
HR 59174CD-2511190142445183931 15 55 30.1-26 15 575.62 A3V
HR 5928ρ5CD-281171414266918395732589846 15 56 53.1-29 12 513.88 B2IV-V 8.838.3G:Sco OB2; Sco-Cen cluster; upper Sco region; member of Pleiades group.
HR 5934BD-20 4364142883183972 7359 15 57 40.4-20 58 595.85 B3V G:Sco OB2; upper Sco complex.,SB:Large amp. Secondary much fainter.,VAR:Beta C?, 5.84 - 5.87V, 0.2872d.
HR 5942CD-2412427142990183982 V913 Sco15 58 34.8-24 49 535.43 B5IV vG:Sco OB2; Sco-Cen cluster; upper Sco region.,RV:vsini 200k/s.,S:He strong?,VAR:Small amp. in y. 0.492d or 0.976d. Also spectrum var.
HR 5944π6CD-25112281430181839875929862 7371 15 58 51.1-26 06 512.89 B1V+B2V 1.20.0C:Color excess E(B-V) = +0.08.,D:Primary is SB, 3.4, 6.4v sep. 0.0003"; third component, ADS 9862B, 12.2v at 50". vsini both A and B =<100k/s.,D:Component B, F4V, optical.,G:Sco OB2; Sco-Cen cluster; in HII region; upper Sco region; member of Pleiades group; in reflection nebula; member assoc.,G:Sco R1 at 145 pc.,SB:ADS 9862A, B1V, B2V, 1.5701d, K 131k/s, V0 -4k/s, msin3i 3.46, asini 2.83. Equal components.
HR 5953δ7BD-22 4068143275184014594IS 16 00 20.0-22 37 182.32 B0.3IV 0.20.2C:Color excess E(B-V) = +0.16. Conspicuous infrared deficiency.,D:Possible quadruple system: SB 3.0, 5.0v, sep. 0.00001", 3.3v at 0.1", and 4.9v at 0.186".,G:Sco OB2; Sco-Cen cluster; upper Sco region; HII region.,N:Dschubba; Iclarkrau.,R:Diam. = 0.00045 - 0.00046".,SB:Primary SB about 20d. Another companion 4.9v at 0.181", discovered by occultation and speckle interferometry, has,SB:longer period. Resolved by speckle observations 1986.45, sep. 0.17".
HR 5965CD-28118171436191840499896 16 02 39.4-29 08 096.03 K3III 6.811.0
HR 5969CD-2511295143787184068I 16 03 20.6-25 51 555.00 K5III G:Probable Hyades group.,R:Occultation diameter measure indicates point source.
HR 5973CD-2412499143900184075I 16 03 54.7-24 43 356.21 K0
HR 5977ξBD-10 42371440691596659909 B16 04 22.1-11 22 235.07 H F5IV 0.21.2D:Binary with HR 5978, q.v.,DYN:0.038".
HR 5978ξBD-10 42371440701596659909 A16 04 22.1-11 22 234.77 H F5IV 0.21.2D:Quintuple system ADS 9909A-C is CPM with ADS 9910, 7.4 G8V, 8.1K0V sep. 11" at 281" from ADS 9909A. ADS 9909AB 4.9 F5IV,,D:4.9 F5IV, 45.69y, a = 0.720". Combined mag. 4.16V, combined colors. ADS 9909C, 7.30V, +0.75(B-V), dG7 at 7", physical.,DYN:0.038".,N:Has been called Grafias, a name more commonly applied to HR 5984.,SB:ADS 9909A, 44.70 yrs. K 3.7k/s, V0 -29.4k/s, asini 549. Period from visual double orbit.
HR 5984β18BD-19 4307144217159682597I9913 A7424 16 05 26.2-19 48 202.62 B1V 1.30.0D:CPM with HR 5985 = ADS 9913C, at 14" and with B, 5.9v at 0.5", possibly SB. Lunar occultations and speckle,D:interferometry indicate companions 4.2v at 0.001" from A and 7.6v at 0.129" from C. Occultations by Jupiter and Io in,D:1971 indicate complex system. Component C occulted by Io revealed the 2.5 mag. fainter companion at 0.1".,DYN:0.004".,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco region.,N:Graffias; Grafias; Grassias; Acrab; Akrab; Elacrab.,R:From occult. by Jupiter, diam. Beta Sco A1 = 0.000422"; diam. Beta Sco A2 = 0.000264".,S:Ca and Na lines nearly stationary.,SB:ADS 9913AD, 6.8281d, K 129.0k/s, V0 -1.0k/s, msin3i 16.0, asini 11.6. Mag. difference about 1v. Apsidal period,SB:51000 times orbital. Unresolved by speckle interferometry. Possible third SB component.
HR 5985β28BD-19 43081442181596839913 C7424 16 05 26.5-19 48 074.92 B2V 1.30.0D:CPM with HR 5984, q.v.,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco region.
HR 5988CD-2312700144334184113 V929 Sco16 06 06.3-23 36 235.92 B8p vG:Sco OB2; Sco-Cen cluster; member of the local association (Pleiades group); upper Sco region.,S:Helium-weak star.,VAR:Spectrum var., amp. 0.03V, 1.49187d.
HR 5993ω19BD-20 4405144470184123 16 06 48.4-20 40 093.96 B1V G:Sco OB2; Sco-Cen cluster; member of the local association (Pleiades group); upper Sco region.
HR 5996BD-13 4342144585159706 16 07 03.4-14 04 156.32 G4IV-V
HR 5997ω210BD-20 4408144608184135I 7454 16 07 24.3-20 52 074.32 G3II-III VAR:Amp. 0.02(b-y).
HR 5998CD-2412552144661184142 16 07 51.9-24 27 436.33 B7IIIp: G:Sco OB2; Sco-Cen cluster; upper Sco region.,S:Helium-weak star.
HR 5999CD-3810893144668207367W CV856 Sco16 08 34.2-39 06 197.05 A7IVe 0.444.1D:CPM with HR 6000 at 44". CD, 7.1, 11.7v, sep. 1.3".,VAR:6.97 - 7.71V, about 30d, variability attributed to circumstellar dust. Possibly a binary shell star with mass exchange.,VAR:Considerable confusion between HR 5999 and 6000 particularly as to which is the variable and which the brighter.,VAR:Originally announced as HR 6000, V856 Sco is really HR 5999, the southern preceding and fainter component C of the,VAR:bright double. The error stems from interchanged photometric data in Harvard Annals 45, 197, 1901, all other early,VAR:visual and photographic estimates indicating that the S. prec. component is the fainter.
HR 6000CD-3810894144667207368W A16 08 34.4-39 05 356.65 A0-3III 0.444.1D:CPM with HR 5999. Component B, 13v at 298".,S:Shell star.,VAR:Not the variable. Originally confused with HR 5999.
HR 6001CD-2511369144690184144I 16 08 07.6-26 19 365.38 M2III
HR 600211BD-12 44251447081597159924 16 07 36.4-12 44 445.78 B9.5Vnn t4.33.5D:CPM.,S:Variable H alpha emission.
HR 6003CD-23127311448441841643275 7470 16 08 43.7-23 41 085.88 B9IVp: G:Sco OB2; Sco-Cen cluster; upper Sco region.,RV:A recent determination of vsini =<15k/s.,S:Helium-weak star.
HR 6006CD-3211456144927207396W 16 09 31.7-32 38 596.19 K0-2III 0.87.7D:Components K0.5IIIab and F4III.
HR 6007CD-33109611449872074033277 16 09 52.6-33 32 455.54 B8V G:Sco-Cen assoc.
HR 6012BD-17 4502145100159745 16 09 55.2-18 20 276.47 F4V
HR 6015CD-40102511451912265643278 16 11 17.7-41 07 115.86 F0IV S:Also classified F2III + (A).
HR 6017CD-2912343145250184197I 16 11 02.0-29 24 595.13 K3III
HR 6026ν14BD-19 43321455011597639951 CD16 11 58.6-19 26 596.30 B8V+B9VpSi 2.541.1D:ADS 9951 at least quintuple system with HR 6027 of which components CD = HR 6026 binary, 6.9 B8V or B9III, 7.9v B9Vp,,D:sep. 2". C is -19d4332.,DYN:0.009".,G:Sco OB2; Sco-Cen cluster; upper Sco member; reflection nebula and dust surrounding star. Assoc. Sco R1; IC 4592 at 145,G:pc.,RV:ADS 9951D, -3k/s; vsini 73k/s.,S:Also classified B9III+B9.5V.
HR 6027ν14BD-19 43331455021597649951 AB16 11 59.7-19 27 384.01 B3V 2.541.1D:ADS 9951A is SB, 4.9, 6.9v, sep. 0.0003". AB, binary. Component B, 6.9v at 1". Components CD at 41" = HR 6026, q.v.,D:HR 6026, q.v.,DYN:0.005".,G:Sco OB2; Sco-Cen assoc.; probable member of Sco-Cen cluster; upper Sco member; in reflection nebula, assoc. Sco R1; IC,G:4592 at 145 pc.,N:Jabbah.,S:H strong; SiIV weak for the spectral type.,SB:ADS 9951A 5.9222d, K 26.4k/s, V0 +1.4k/s, asini 2.15.
HR 602813CD-2710841145482184221 16 12 18.2-27 55 354.59 B2V G:Sco OB2; Sco-Cen cluster? Upper Sco region; embedded in reflection nebulosity.
HR 602912CD-28119621454831842179953 7520 16 12 15.9-28 25 035.67 B9V v2.13.9D:Binary, companion F3V.,G:Sco OB2; upper Sco region.
HR 6031ψ15BD-09 43241455701410223280 16 12 00.0-10 03 514.94 A3IV N:Some early catalogues (particlarly BAC) call Flamsteed 15 Chi instead of Psi Sco and leave 17 (HR 6048 =,N:Chi) unnumbered. All later sources adopt the convention followed here.
HR 603316BD-08 4180145607141024 16 12 07.3-08 32 515.43 A4V
HR 6042CD-24126231457921842419967 16 13 45.7-24 25 196.41 B5V 3.81.5G:Sco OB2; Sco-Cen assoc.; upper Sco region; Sco-Cen cluster.
HR 6044CD-3211525145838207480 16 14 22.3-33 00 415.92 K0III
HR 6048χ17BD-11 4096145897159793I 16 13 50.9-11 50 155.22 K3III N:See HR 6031.
HR 6051BD-20 4444145964184253 16 14 28.8-21 06 276.41 A0V
HR 6053BD-18 4249145997159807D 16 14 39.1-18 32 076.32 K2III 0.30.0D:Sep. 0.03".
HR 6054CD-2511453146001184258 16 14 53.6-25 28 376.05 B7IV G:Sco OB2; Sco-Cen cluster; upper Sco region.
HR 606018BD-07 4242146233141066W 7577 16 15 37.3-08 22 105.50 G2Va 7.725.8D:Optical.
HR 6061BD-14 43831462541598213286 7578 16 15 51.5-14 50 576.09 A0V
HR 6066BD-20 4454146416184285 16 16 58.8-21 18 146.61 B9V G:Sco OB2; Sco-Cen cluster; upper Sco region.
HR 6070CD-28120371466241843013288 16 18 17.9-28 36 504.78 A0V
HR 6076BD-19 4357146834184309 16 19 07.7-20 13 046.29 K5III C:UBV photometry indicates strong interstellar absorption, confirmed by neighboring stars. However, the spectral type is,C:considerably later than expected, even from the observed (B-V).,G:UMa stream; in reflection nebula; assoc. Sco R1. If a member of UMa stream, it must be an interloper in the upper Sco,G:nebulosities.,S:Variously classified G5III, G8IIIb, K0.5III and K5III.
HR 6077CD-30130411468362075581426W A16 19 32.7-30 54 245.49 F6III 1.623.2D:Companion, F9V, CPM.,SB:Component A of visual double.
HR 6078BD-14 4398146850159846I 16 19 00.4-14 52 215.94 K4III
HR 6080CD-3910412146954207574W 16 20 32.6-39 25 516.12 B9V 4.715.6
HR 6081ο19CD-2312849147084184329I 7632 16 20 38.2-24 10 104.55 A5II vC:Probably not IR source. Heavily reddened. Analysis of spectral energy distribution (Whittet 1988, MNRAS, 230, 473),C:shows no significant IR excess and possible overluminosity for A5II type.,G:Sco-Cen assoc.; upper Sco complex.,VAR:Small amp. in V. MgII 4481 appears to vary.
HR 6084σ20CD-2511485147165184336607I10009 Sig Sco16 21 11.3-25 35 342.89 B1III 2.00.0C:Color excess E(B-V) = +0.40. Reddened star.,D:B, 8.26V, +0.25(B-V), -0.23(U-B), B9.5V at 20", optical; vsini : 54k/s. The visual primary is triple: SB, 3.3, 5.3v,,D:sep. 0.0005" and 5.5v at 0.49", discovered by occultation.,G:Sco OB2; Sco-Cen cluster; upper Sco region; HII region S9; in reflection nebula; assoc. Sco R1.,N:Alniyat; Al Niyat. Name applies to pair with HR 6165.,RV:ADS 10009B, -6k/s.,S:Stationary Ca lines. Although this star is an MK standard for class B1III, it is a variable, a multiple star, and is,S:situated in reflection nebulosity. Component A has also been classified as B2III and B2IV; component B as B9V, B9.5V,,S:and B8Vp. From scanner studies of composite spectra, Beavers (ApJS, 44, 489, 1980) finds ADS 10009A can be,S:resolved into O9.5 and B7 with a magnitude difference of 1.6V.,SB:ADS 10009A, 34.23d, K 34.0k/s, V0 +2.5k/s, asini 14.9.,VAR:Beta C 2.94 - 3.06B. Multiple periods, 0.2468429, 0.239671, 8.2, and 33.1d. Surrounded by HII region. Primary,VAR:period varies in period of 23.2y with an amp. of 0.7 sec. Occultations indicate the variable has a 2.2 mag. fainter,VAR:companion at 0".49. The duplicity had been suspected from occultations as early as 1860. Orbital period probably over,VAR:112 yrs. UV observations indicate temperature varies by 2510K and ratio max. to min. radius by 1.095.
HR 6094CD-38109831475132076223295 7680 16 24 01.3-39 11 355.40 G5V VAR:Amp. 0.07V.
HR 6097CD-3211687147553207625W A16 23 56.7-33 11 586.47 A0V+A0V 0.56.3D:Components also classified B9.5V(n) and A1V(n).
HR 6100CD-3710778147628207637W 16 24 31.7-37 33 575.42 B8IV 0.10.1D:Sep. 0.098".,G:Sco-Cen assoc.
HR 6105CD-291251314772218436810035 B16 24 39.6-29 42 126.63 G0IV 0.85.2D:Binary with HR 6106, q.v.
HR 6106CD-291251314772318436910035 A16 24 39.7-29 42 175.84 G0IV 0.85.2D:Binary with HR 6105. Mag. and colors for combined light, 5.41V, +0.59(B-V), +0.12(U-B).
HR 6122CD-3610783148247207688 16 28 14.7-37 10 465.79 K1IIICNII
HR 6134α21CD-2611359148478184415616I10074 Alp Sco16 29 24.4-26 25 550.96 M1.5Iab-Ib+B4Ve 4.22.9D:Var. M1Ib, 5.5 B2.5V, 878y, a = 2.90", masses 15.5 and 7.0 solar. Companion is radio source. SKYLAB confirms cool star,,D:hot companion.,DYN:0.011".,G:Sco OB2; Sco-Cen stream; in reflection nebula; assoc. Sco R1; dust shell beyond 12 R.,N:ANTARES; Cor Scorpii; Kalb al Akrab; Vespertilio.,R:Occultation diam. = 0.041".,RV:7.5 yrs.,S:Ultraviolet FeII emission. 5-micrometer observations indicate carbon monoxide.,VAR:ADS 10074A, SRc 0.88 - 1.8V, 1733d. Possibly considerably fainter before 150 A.D.: see HR 5685.
HR 614122CD-2412695148605184429 16 30 12.4-25 06 544.79 B2V G:Sco OB2; probable member of Sco-Cen cluster, upper Sco region; in reflection nebula; assoc. Sco R1; IC 4605.
HR 6142CD-4110695148688226855W 7781 16 31 41.7-41 49 015.33 B1Iae v4.358.0D:Components A (F5V) and B both optical.,S:Oxygen-rich supergiant.,VAR:Spectrum variable?
HR 6143CD-34110441487032077321431 16 31 22.9-34 42 164.23 B2III-IV G:Sco-Cen cluster.
HR 6145CD-2611379148760184437 16 31 22.8-26 32 166.10 K1III
HR 6160CD-4410964149174226926 7829 16 35 07.9-45 14 416.46 K2-3III VAR:Amp. 0.08V.
HR 6164CD-4211399149404226953 V918 Sco16 36 22.5-42 51 325.47 O9Ia eG:Ara OB1a. Listed by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) as among Sco-Cen stars. Buscombe now points out,G:that it is a nonmember background star.,RV:Two available determinations of vsini, 140 and 45k/s.,S:H alpha emission.,SB:9.813d, k1 101k/s, K2 60k/s, V1 -37k/s, V2 -28k/s, m1sin3i 1.6, m2sin3i 2.7,,SB:a1sini 13.7, a2sini 8.1.
HR 6165τ23CD-2711015149438184481620 16 35 53.0-28 12 582.82 B0V C:Color excess E(B-V) = +0.06.,G:Sco OB2; Sco-Cen cluster; Sco-Cen assoc.; upper Sco region. Faint HII region surrounds star. Member of Pleiades group.,N:See HR 6084.,S:Spectra indicate high velocity stellar wind. Lyman beta observed from COPERNICUS. High resolution UV spectrum,S:obtained from COPERNICUS. Large amount of atomic hydrogen, but only small amount of molecular hydrogen in line of sight.
HR 6166CD-3411112149447207814I 7844 16 36 22.5-35 15 204.16 K6III
HR 6174CD-4310959149711226989W 16 38 26.2-43 23 555.83 B2.5IV 3.216.3D:CPM.,G:Member of the local association (Pleiades group); Sco-Cen assoc.
HR 6178CD-36108791498862078783317W 16 39 05.2-37 13 035.91 B9-A0V+B 0.00.1D:Sep. AB, 0.102".
HR 6192CD-3211913150331207930 16 41 45.5-33 08 475.87 G3III
HR 6206CD-4010649150573227118W 16 43 45.5-41 07 086.20 A4V 0.195.7D:CPM with HR 6209 at 96".,G:Sco OB1.
HR 6209CD-4010653150591227123W 16 43 53.9-41 06 476.12 B6-7V 0.195.7D:CPM with HR 6206.,G:Sco OB1.
HR 6210CD-3710942150608207966W 16 43 47.6-38 09 246.05 B9II-III 6.250.0
HR 6211CD-31131611506382079673325 16 43 38.7-32 06 226.46 B8V
HR 6214CD-40106611507422271463329W 16 44 42.6-40 50 235.71 B3V 6.38. D:Secondary A5V, optical.,G:Member of the local association (Pleiades group); Sco OB1.
HR 6216CD-271110315076818459110173 7935 16 44 17.3-27 27 226.58 A2V 4.02.0D:ADS 10173AB, binary.,VAR:E?, amp. 0.03V.
HR 6218CD-2812358150894184602W 7944 16 45 00.2-28 30 356.02 A3IV 7.75.6
HR 6221CD-3910677151078208020 16 46 47.8-39 22 385.48 K0III
HR 622525CD-2511667151179184630 16 46 51.3-25 31 436.71 gG6
HR 6241ε26CD-3411285151680208078628 7983 16 50 09.8-34 17 362.29 K2.5III
HR 6244CD-3711023151771208089W Var?16 50 59.8-37 30 526.11 B9pSi* 2.26.7RV:Companion -30k/s, double lines velocity separation 258k/s, both components B9V.,S:Also classified B8II/III.,VAR:Long per?
HR 6245CD-4110957151804227313 7992 16 51 33.7-41 13 505.22 O8Iaf G:Sco OB1. Possible member of open cluster NGC 6231, 30' south of the center. See HR 6260.,RV:Outward moving atmosphere.,S:Shell star.
HR 6247μ1CD-37110331518902081021439 Mu1 Sco16 51 52.2-38 02 513.08 B1.5V+B6.5V 0.4390. D:CPM with HR 6252 at 346".,G:Sco-Cen cluster; Sco-Cen assoc.; upper Sco; member of Pleiades group.,SB:1.4463d, K 185k/s, V0 0k/s, msin3i 9.09, asini 3.68. Equal components. Semi-detached system.,VAR:EB 2.80 - 3.08B, 1.44026907d. Semi-detached system.
HR 6249CD-4110972151932227328I V919 Sco16 52 19.1-41 51 166.49 WN7-A C:Strongly reddened.,G:Sco OB1; HII region; member NGC 6231. See HR 6260.,RV:3.5d not confirmed.,S:Circumstellar matter. Helium rich. The A in the spectral type here means narrow lines, not an A-type spectrum.,VAR:6.51 - 6.61V, HeI, NII 4097 var. 3.5d.
HR 6252μ2CD-3711037151985208116 16 52 20.1-38 01 033.57 B2IV 0.4390. D:CPM with 6247 at 346".,G:Sco-Cen cluster; Sco-Cen assoc.; upper Sco; member of Pleiades group.
HR 6257CD-4211627152161227359 8012 16 53 42.5-43 03 035.96 M3II-III VAR:Amp. 0.14V.
HR 6260CD-4111024152234227377W 16 54 01.8-41 48 235.45 B0.5Ia 1.50.4D:Component F, 7.3v O6, vsini 125k/s.,G:NGC 6231 #290. The open cluster NGC 6231 is the nucleus of Sco OB1 assoc., which is surrounded by an elliptical HII,G:region extending 4d or 5d. Diam. of cluster 26'. Considerable dark nebulosity close to cluster. HR 6245, 6249, 6261 and,G:6265 also in the cluster.,S:Nitrogen deficient.
HR 6261CD-4111021152235227374 V900 Sco16 53 58.8-41 59 416.32 B1Ia eC:Strongly reddened.,G:Sco OB1; in cluster NGC 6231. See HR 6260.,S:H alpha emission. Nitrogen deficient. Strong OII.,VAR:6.29 - 6.34V, 2.631? or 6.28 or 6.85d.
HR 6262ζ1CD-4211633152236227375 Zet1 Sco16 53 59.7-42 21 444.73 B1Iape vC:Strongly reddened.,G:Possible member of NGC 6231, 30' south of the center of the cluster. See HR 6260.,RV:Mass loss estimated 0.00005 solar masses/y.,S:Shell star. Possible H alpha emission.,VAR:Amp. 0.09V. Variations in HeI, NII, OII suggest turbulent outer layers.
HR 6263CD-4111036152249227383 8023 16 54 11.8-41 51 016.45 O9Ib G:Sco OB1; in open cluster NGC 6231 #293. See HR 6260.,S:Also classified OC9.5Iab, OC9.5I and O9.5I.,SB:5.97d, K1 191k/s, K2 206k/s, V1 -44k/s, V2 -8k/s, msin3i 20.1, asini 15.7.,VAR:6.34 - 6.50V.
HR 6265CD-4111041152270227390W Var?16 54 19.6-41 49 126.59 WC7+O5-8 6.64.3C:Strongly reddened.,D:Innes and IDS data on components and number of components appear inconsistent. Probably different cluster components,D:measured.,G:In cluster NGC 6231 #220. See HR 6260.,RV:Shell of WR component expanding at 1688k/s.,SB:Component A of visual double, 8.893d, K 142k/s, V0 -27.2k/s, msin3i 1.75, asini 17.4. Same period for both,SB:absorption and emission lines, but differ in phase by 0.5 period.
HR 6266CD-4211642152293227392 16 54 26.9-42 28 445.88 F5Ib-II G:Sco OB1.
HR 6271ζ2CD-4211646152334227402 8028 16 54 35.0-42 21 413.62 K4III G:Sco OB1.,VAR:3.6 - 3.64V.
HR 6272CD-4010919152408227425W 8031 16 54 58.4-41 09 045.77 O8:Iafpe 7.05.4D:Companion F4p.,G:Runaway star from Sco OB1. Possible member NGC 6231, 30' south of the center of the cluster. See HR 6260.,M:Either runaway, or P Cyg type with extended expanding atmosphere.,RV:Mass loss 0.00009 solar masses/y.,S:Shell star. Sp. shows interstellar Lambda4430.,VAR:Amp. 0.07V.
HR 6273CD-3013594152431208176 16 54 36.0-30 35 146.35 A7IIIm:
HR 6282CD-3311570152636208205 16 55 57.8-33 30 266.37 K5III
HR 6283CD-4010975152667227473 V861 Sco16 56 36.0-40 49 256.15 B0.5Ia eC:Strongly reddened.,G:In cluster Collinder 316; Sco OB1.,RV:Also 0.6147d related to rotation of primary. Mass loss 0.000027 solar masses/y.,S:H alpha emission. Nitrogen deficient. P Cyg type?,SB:7.8483d, K 84.5k/s, V0 -34.6k/s, asini 9.09. Alternate orbits 7.8483d, K 99.4k/s, V0 -43.3k/s; 7.848250d,,SB:K 82k/s, V0 -31k/s; 7.84825d, K 87.3k/s, V0 -34.4k/s, asini 9.4. Low mass companion. Tidal distortion.,VAR:EB 6.07 - 6.69V, 7.84818d.
HR 628827CD-3311590152820208232 16 57 11.1-33 15 345.48 K5III
HR 6298CD-3711131153072208259W 16 58 52.4-37 37 166.09 A3V 0.20.2D:6.7 A3V, 6.9 A4V, 37.9y, a = 0.181". Combined mag., colors.
HR 6303CD-4511123153258227547 17 00 32.3-45 27 066.65 K4III
HR 6311CD-3511236153368208293 17 00 36.9-35 56 035.97 K2IIICNII
HR 6316CD-31134731536132083243354W 17 01 52.7-32 08 375.03 B8V 7.523.8D:All companions optical. B is A8V, C is F5V.,G:Sco-Cen assoc.
HR 6327CD-3711201153890208355 V923 Sco17 03 50.8-38 09 085.91 F4IV+F2V G:NGC 6281 #1 (nonmember).,SB:34.8189d, K 53.6k/s, V0 -14.8k/s, msin3i 1.48, asini 23.3.,VAR:E amp. 0.35V, 34.8269:d.
HR 6331CD-4511188154025227601 17 05 05.3-45 30 066.28 A2V
HR 6334CD-3311706154090208377W 17 04 49.4-34 07 224.87 B1Ia t9.120. G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster.,VAR:H alpha profile variable.
HR 6338CD-4311396154153227615 17 05 48.6-44 06 186.19 A4III
HR 6344CD-3711274154310208406W 17 06 20.3-37 13 395.98 A2IV 4.95.8
HR 6347CD-3511306154368208410W 17 06 28.4-35 27 046.13 O9.5Iab 6.52.8C:B-V values scatter from +0.38 to +0.60, U-B from -0.37 to -0.63.,G:Sco OB4. Listed by Buscombe and Kennedy (M.N.R.A.S. 124, 196, 1962) as among Sco-Cen stars. Buscombe now points out,G:that it is a nonmember background star.,S:Strong interstellar lines indicate the interstellar molecules CH, CH+, and CN are in localized area near the Sun.
HR 6366CD-30138401547832084673363 17 08 47.5-30 24 135.97 A/FmDel Del G:Hyades group.,S:Also classified F0III.
HR 6371CD-4411502154948227688W 17 10 42.3-44 33 275.08 G8-K0III+G 7.913.2
HR 6380ηCD-4311485155203227707638 17 12 09.2-43 14 213.33 F3III-IVp G:Hyades group.,S:Also classified F2V.
HR 6381CD-39111821552592085213366 17 12 16.2-39 30 255.67 A1V
HR 6382CD-3811632155276208522 17 12 16.5-38 49 206.30 K1IIICNII
HR 6389CD-3212460155450208539W 17 12 58.7-32 26 196.01 B1II 7.530. G:Sco OB4; doubtful member of the Sco-Cen cluster; possible new OB assoc. in Sco with HR 6397 and HR 6422.
HR 6392CD-3911212155603208569IW V915 Sco17 14 27.7-39 46 016.60 G5Ia 4.214.4D:Component B, 10.42V, +0.52(B-V); component C, 11.40V, +1.55(B-V).,VAR:Amp. 0.15V.
HR 6397CD-3311875155806208585 8388 17 15 19.3-33 32 545.53 O7.5V[n]e G:Sco OB4 assoc.; possible new OB assoc. in Sco with HR 6389 and HR 6422.,S:Variously classified O5pe, O7.5-O8IIIe, O7.5Vne, O8-O9Ve.,VAR:Emission lines variable? H alpha width and profile vary.
HR 6398CD-3811686155826208591W 17 15 35.9-38 35 385.96 F7V+G2V 0.10.1D:Sep. 0.108". Speckle observations 1986.45 give 0.14".
HR 6403CD-3013968155940208606 17 15 51.5-30 12 386.21 B9.5V
HR 6405CD-3511426155974208610W 17 16 21.5-35 44 586.12 G0IV-V 7.436.5
HR 6409CD-32125451560982086261452 17 17 03.7-32 39 465.55 F6IV G:Hyades group.
HR 6420CD-4311572156293227813 17 18 48.0-44 07 475.76 B9V
HR 6422CD-3212573156325208657W Var?17 18 20.4-32 33 126.36 B5Vn e5.619.5D:Companion is F2V.,G:Sco OB4; Sco-Cen assoc. See HR 6389.,VAR:Amp. 0.04V on time scale 3 hrs. and 0.05 on time scale 1d suspected.
HR 6426CD-3411626156384208670W 8482 17 18 57.2-34 59 235.91 K3V+K5V 1.00.5D:AB 6.1 K3V, 7.6 K5V, 42.177y, a = 1.734" or 42.09y, a = 1.82", combined mag., colors. Component C, 9.9v M2, 32",D:physical. D, 12.8v at 15".,DYN:0.144".,VAR:Amp. 0.04.
HR 6427CD-4411595156398227821W 17 19 24.5-44 13 236.65 B9.5V+A6III 0.30.2D:Binary. Combined mag., colors, sep. 0.200".
HR 6450CD-3711507157038208740W 17 22 39.4-37 48 186.41 B4Ia 5.82.7C:V magnitudes scatter from 6.31 to 6.44, B-V from +0.61 to +0.89, U-B from +0.01 to -0.30.,G:Sco-Cen assoc.; in HII region.,S:NII and MgII indicate different spectral classes. Component B is G type.
HR 6454CD-3511505157060208741 17 22 38.0-35 54 366.47 F7V
HR 6456CD-3711512157097208747W 17 22 54.9-37 13 145.93 K1III 8.420.2
HR 6460CD-4411669157243227911 17 24 13.0-44 09 455.12 B7III G:Sco-Cen assoc.
HR 6470CD-3411674157486208786 17 25 02.7-34 41 476.16 A0VSiCr
HR 6501CD-3611546158105208860 17 28 56.1-36 46 426.02 K0III
HR 6503CD-3811927158156208870W 17 29 25.7-38 31 006.39 A2V 0.30.4
HR 6508υ34CD-3711638158408208896649 17 30 45.8-37 17 452.69 B2IV C:Color excess E(B-V) = +0.02.,G:Sco-Cen assoc.,N:Lesath; Lesuth.,S:Lyman alpha and Lyman beta observed from COPERNICUS.
HR 6517CD-3312149158619208921 17 31 47.4-33 42 106.44 K2III
HR 6522CD-3411757158741208935 V949 Sco17 32 24.5-34 16 476.17 F2V
HR 6523CD-4111742158799228110 17 33 07.4-41 10 255.84 B9Ib-II
HR 6527λ35CD-3711673158926208954652W Lam Sco17 33 36.5-37 06 141.63 B2IV+B 10.394.9C:Color excess E(B-V) = +0.03.,G:Sco-Cen assoc.,N:SHAULA.,S:Lyman alpha and Lyman beta observed from COPERNICUS.,SB:5.6d. Interferometer measures indicate multiple star.,VAR:Beta C 1.59 - 1.65V, 0.2137015d, secondary 0.1068518d, beat period 10.1605d. Also possible 0.04V eclipse. X-ray,VAR:flare observed in vicinity Lambda Sco on 1 June 1975.
HR 6535CD-3212935159176208977W 9167 17 34 42.5-32 34 545.70 O7V+O7V 4.85.4D:Component B, B9V; C, B8V.,G:In cluster NGC 6383 #1; in HII reg. Ma 322; in nebulosity. Embedded in large neutral hydrogen complex of which a small,G:part is ionized by the hot O7-type star.,M:Central star of open cluster NGC 6383, probably older than the rest of the cluster core and might have initiated star,M:formation in the core and beyond.,SB:3.3666d, K 213.8k/s, V0 +9.1k/s, msin3i 12.7, asini 9.90. Two O7V components, about 30 solar masses. vsini of,SB:secondary 148k/s.,VAR:Ell?, 5.68 - 5.71V.
HR 6539CD-3711702159312209001 17 35 43.0-37 26 246.48 A0V
HR 6546CD-3812044159433209019 9205 17 36 32.8-38 38 074.29 K0IIIb
HR 6553θCD-4212312159532228201654 9233 17 37 19.2-42 59 521.87 F1II N:Sargas.,VAR:1.90 - 1.94V?
HR 6557CD-3711723159633209034 17 37 26.8-38 03 566.26 G2Ib
HR 6558CD-4212327159707228220 17 38 08.5-42 52 506.10 B8V
HR 6580κCD-3812137160578209163660 Kap Sco17 42 29.3-39 01 482.41 B1.5III G:Sco-Cen assoc.,SB:Same periods as VAR.,VAR:Beta C 2.39 - 2.42V, 0.1998303d, 0.205430, 7.3316, 0.189512 and 2.591d.
HR 6583CD-3611804160668209172 17 42 51.0-36 56 455.54 K5III
HR 6587CD-3213208160748209176 17 43 06.9-33 03 046.40 M1III
HR 6597CD-4212431160928228363W 17 44 42.0-42 43 445.87 A1V+F0IV 0.10.1D:Sep. 0.111".
HR 6613CD-3812189161390209246W 17 47 07.3-38 06 426.43 B9V+A1V 0.30.1D:7.1 B9, 7.3, 34.00y, a = 0.157". Combined mag., color.
HR 6615ι1CD-4011838161471228420666W 17 47 35.1-40 07 373.03 F2Iae 9.937.5
HR 6628CD-3114609161840209303 17 49 10.5-31 42 124.83 B8V
HR 6630CD-3711907161892209318669W 17 49 51.5-37 02 363.21 K2III 11.541.7
HR 6631ι2CD-4011886161912228466W 17 50 11.2-40 05 264.81 A2Ib 6.132.6
HR 6643CD-4011905162189228489W 17 51 32.8-40 46 215.96 M2III 6.523.6
HR 6645CD-3014802162220209357W 17 51 12.5-30 33 266.66 A0Vn 1.510.2D:Companion A0IV. Fixed sep.
HR 6647CD-3412165162374209383 V957 Sco17 52 13.6-34 47 575.90 B6V vG:Open cluster NGC 6475 #26; M7 blue straggler.,RV:He lines show var. RV; H, Mg, Si do not.,VAR:SX Ari, amp. 0.05V, 1.658d. Spectrum variable.
HR 6648CD-3412170162391209390 17 52 19.7-34 25 005.84 G8III
HR 6649CD-4112139162396228510 17 52 52.7-41 59 486.20 F8IV-V
HR 6651CD-3412186162496209397 17 52 49.2-34 06 516.06 K1III
HR 6652CD-3412187162515209401 17 52 55.9-35 01 076.45 B9.5V G:Open cluster NGC 6475 #42; M7.,SB:6.67683d, K 57.6k/s, V0 -8.7k/s, asini 5.29. Alternate orbit 6.6768d, K 53.4k/s, V0 -12.3k/s, asini 4.90.,SB:Secondary much fainter.
HR 6653CD-3512013162517209404 17 52 57.9-35 37 276.03 F2III-IV
HR 6657CD-3412200162586209411W 17 53 19.6-34 43 506.17 B8V 0.00.1D:6.9, 6.9v, 160.759y, a = 0.37".,G:Open cluster NGC 6475 #56.
HR 6658CD-3412203162587209416W 17 53 23.3-34 53 435.60 K3III 0.10.4D:Binary.,G:Open cluster NGC 6475 #58.
HR 6660CD-3412219162678209425 17 53 45.5-34 47 096.38 B9V G:NGC 6475 #141.
HR 6662CD-3412226162724209428W V906 Sco17 53 54.9-34 45 095.96 B9V+B9V 0.80.3G:Sco-Cen assoc.; open cluster NGC 6475 #86.,SB:2.7754d, K 121k/s, V0 -32k/s, msin3i 3.15, asini 4.54. Triple-lined SB. vsini of secondary 50k/s.,VAR:E? Amp. 0.26V.
HR 6663CD-3412228162725209430 V951 Sco17 53 58.1-34 49 546.42 ApSi* G:Open cluster NGC 6475 #88.,S:Also classified A0VpSiCr, B9Si, and B9III.,VAR:Amp. 0.04V. Possible periods 4.45597, 4.4588d (North 1984, A&AS, 55, 259).
HR 6668CD-3412244162817209446 17 54 27.2-34 27 595.96 B9.5V G:NGC 6475 #110.
HR 6671CD-3612008162926209458 17 55 07.9-36 28 336.06 B9.5III
HR 6675CD-44122011631452285623425 17 56 47.4-44 20 324.86 K2III
HR 6678CD-4012001163234228564 17 56 55.8-40 18 206.43 K3III
HR 6682CD-4112231163376228578 17 57 47.7-41 42 584.88 M0III
HR 6683CD-3912058163433209524W 17 57 57.8-39 08 136.29 A0IV-V 1.50.7

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetary Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 607216 12 58.2-36 13 46PN14.111.71.63pF, R, vgvlbM, rPK 342+10.1, ESO 389-PN15, AM 1609-360, CS=17.5
NGC 615316 31 30.6-40 15 11PN11.510.90.4planetary, stellarPK 341+5.1, ESO 331-PN6, AM 1628-400
NGC 630217 13 44.1-37 06 12PN12.89.61.48pB, E pf (Swift: triple)PK 349+1.1, ESO 392-PN5, Sh2-6, Bug nebula
NGC 633717 22 15.7-38 28 59PN11.912.30.85!!! annular, eF, S, am stPK 349-1.1, ESO 333-PN5, AM 1718-382, CS=14.8
IC 459916 19 23.2-42 15 34PN12.40.25Planetary, 15 magPK 338+5.1, ESO 331-PN1, AM 1615-420
IC 463717 05 10.4-40 53 05PN13.612.50.37Planetary, stellarPK 345+0.1, ESO 332-PN21, CS=12.3
IC 466317 45 28.7-44 54 16PN13.112.50.33Planetary, stellPK 346-8.1, ESO 279-PN6, CS=14.0
Galactic Nebulae
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 633417 20 48.0-36 06 12EN35 × 20cF, vL, icE, vglbf, * 8 invESO 392-EN9, Sh2-8, CED 140
NGC 635717 24 43.5-34 12 05EN+OCL25 × 25F, L, E, vglbM, D * invESO 392-SC10, CED 142, Sh2-11
IC 459116 12 18.0-27 55 40RN+*12 × 10* 5.6 in F nebLBN 1096, ESO 451-*N16
IC 459216 11 59.6-19 27 35RN+*150 × 60vL, E, ν2 Scorpii invLBN 1113, ESO 584-N*6, CED 128
IC 460116 20 18.0-20 04 54RN+*20 × 102 st 8 in eL, dif neb, lE npsfESO 585-*N1, CED 129C
IC 460516 30 12.5-25 06 53RN+*30 × 30* 7 in eF, vL nebLBN 1110, ESO 517-*N8, CED 133
IC 462816 57 00.0-40 27 24EN90 × 60F, eL, E pf, difESO 332-EN14
Open Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 612416 25 17.2-40 40 01II3m5.840Cl, B, L, pRi, lCM, st 9…11OCL 990, ESO 331-SC3
NGC 617816 35 50.8-45 38 48I3p7.25Cl, B, S, st pLOCL 980, ESO 276-SC6
NGC 619216 40 20.8-43 21 55I2p8.59Cl, pL, pRi, iR, st 11…14OCL 988, ESO 277-SC3
NGC 621616 49 23.5-44 43 53II2p10.14Cl, pS, pRi, pC, st 12…15OCL 989, ESO 277-SC14
NGC 623116 54 09.8-41 49 30I3p2.82.614Cl, B, cL, pRi, st 10…13OCL 997, ESO 332-SC6
NGC 624216 55 30.6-39 28 01I3m6.49Cl, B, L, Ri, st 8…11OCL 1001, ESO 332-SC10
NGC 624916 57 41.7-44 48 17II1p8.26Cl, pRi, vlC, iF, st L & SOCL 994, ESO 277-SC19
NGC 625917 00 45.3-44 39 18III2m8.015! Cl, B, vL, vRi, st 11…NGC 6222, OCL 996, ESO 277-SC22
NGC 626817 02 04.1-39 43 16II2p9.56Cl, B, pL, cRi, st 10…OCL 1002, ESO 332-SC17
NGC 628117 04 47.2-37 53 16II2p5.48Cl, L, pRi, lC, st 9…11OCL 1003, ESO 332-SC19
NGC 631817 16 13.4-39 25 26III2p11.85Cl, pL, Ri, R, gbM, st 12…14OCL 1004, ESO 333-SC1
NGC 632217 18 25.7-42 56 02I2p6.05Cl, vL, pRi, lC (place of * nf)OCL 1000, ESO 278-SC6
NGC 638317 34 42.2-32 34 54IV3p5.65.520Cl, st 13, * 6·7 in MNGC 6374, OCL 1026, ESO 393-SC7
NGC 639617 37 36.2-35 01 33II3p8.53Cl, pL, lRi, lCOCL 1018, ESO 393-SC10
NGC 640017 40 12.0-36 57 42II2m8.812Cl, pL, pRi, iR, st 9…10OCL 1014, ESO 393-SC14
NGC 640417 39 37.3-33 14 48III3m10.66Cl, F, L, pRi, lC, st 13…15OCL 1024, ESO 393-SC13
NGC 640517 40 20.0-32 15 30III2p4.54.233Cl, L, iR, lC, st 7, 10…M 6, OCL 1030, ESO 455-SC30, Butterfly cluster
NGC 641617 44 19.9-32 21 40IV1p5.715Cl, vL, Ri, lCOCL 1031, ESO 455-SC32
NGC 642517 47 00.0-31 31 48I1p7.210Cl, pS, lRi, lC, st 10…12OCL 1033, ESO 455-SC38
NGC 644417 49 35.1-34 49 11III2m12Cl, vL, vRi, st 12…13OCL 1023, ESO 393-SC30
NGC 645117 50 40.5-30 12 42II1p8.28Cl, pL, pRi, bifid, st 12…OCL 1035, ESO 455-SC50
NGC 647517 53 50.0-34 47 36II2r3.53.375Cl, vB, pRi, lC, st 7…12M 7, OCL 1028, ESO 394-SC9, Ptolemy's cluster
Globular Clusters
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 609316 17 02.5-22 58 28II7.310!! globular, vB, L, vmbM (var *), rrr, st 14M 80, GCL 39, ESO 516-SC11
NGC 612116 23 35.5-26 31 29IX5.436Cl, 8 or 10 B st in line, with 5 st, rrrM 4, GCL 41, ESO 517-SC1
NGC 613916 27 40.4-38 50 54II9.18.2B, pL, R, psbM, rrGCL 43, ESO 331-SC4
NGC 614416 27 14.1-26 01 27XI9.07.4Cl, cL, mC, gbM, rrrIC 4606, GCL 42, ESO 517-SC6
NGC 625616 59 32.6-37 07 15GCL11.34.1globular, vF, vL, iR, vgbM, rrrGCL 49.1, ESO 391-SC6, vdB-Hagen 208
NGC 638017 34 28.0-39 04 07GCL11.53.6eF, pS, lE, * 9 attGCL 68, ESO 333-SC14
NGC 638817 36 17.0-44 44 04III6.810.4globular, vB, L, R, pg, psvmbM, rrr, st 17…GCL 70, ESO 279-SC2
NGC 644117 50 12.9-37 03 02III7.29.6globular, vB, pL, R, vgmbM, rrr, st 18GCL 78, ESO 393-SC34
NGC 645317 50 51.8-34 35 53IV10.27.6cL, iR, pmbM, rGCL 79, ESO 393-SC36
NGC 649617 59 02.0-44 15 52XII8.65.6Neb + Cl, pL, mE, gvlbMGCL 80, ESO 279-SC13
Galaxies
NameRADecTypebMagvMagDimDreyer DescriptionIdentification, Remarks
NGC 600015 49 49.4-29 23 13SBbc12.711.91.9 × 1.6vF, S, R, sbMESO 450-20, MCG -5-37-3, IRAS 15467-2914
IC 459616 16 03.6-22 37 29SBab14.814.01.5 × 0.5F, S, mE 40°, mbMN, prob spirESO 516-9, MCG -4-38-5
IC 459716 17 39.7-34 21 58S0-a14.613.71.2 × 1bM, magn 14ESO 380-2, IRAS 16144-3414
IC 459816 18 13.2-31 26 29Sbc14.613.81.5 × 0.4Neb streak of F st, 1' nsESO 451-18, IRAS 16150-3119
IC 460016 16 05.3-22 46 59S0-a16.415.50.4 × 0.4eF, eS, RESO 516-10

«Strasbourg-ESO Catalogue of Galactic Planetary Nebulae» Acker et al., 1992 [141]
PNGRADecMain IDPKIRASDiscovererIdentitiesoDiam
["]
rDiam
["]
Dist
[kpc]
Rvel
[km/s]
ExpVel
[km/s]
C* NameC* MagC* SP Type
PN G000.3-02.817 57 42-30 02 02M 3-470-02.5MINKOWSKI 1948ESO 456-22, Sa 3-100, VV' 296 0. -16.0 ± 5.0
PN G000.5-03.117 59 16-30 02 48KFL 1KINMAN et al 1988 8.2 -51.0B: 18.4, V: 17.3
PN G338.8+05.616 19 23-42 15 36He 2-155338+05.116158-4208HENIZE 1964Sa 2-141, ESO 331-01, Wray 16- 215 14.5 -26.5 ± 8.8B: 16.7, V: 16.3
PN G341.8+05.416 31 31-40 15 22NGC 6153341+05.116280-4008COPELAND 1883ARO 501, ESO 331-06, He 2- 167, RCW 112, Sa 2- 148, VV 81, VV' 141, Wray 16-225 24. 1.8 +37.0 ± 3.0 17.5 (O-III), 17. (N-II)AG82 210bis, CD -39 10464, GCRV 9495, HD 148687B: 16.14
PN G342.1+10.816 12 59-36 13 39NGC 6072342+10.116097-3606HUBBLE 1921ARO 500, ESO 389-15, My 93, Sa 2- 134, VV 77 70. 1.9 +7.0 ± 2.0< 6.0 (O-III), 10.0 (N-II)AG82 200B: 19.31
PN G342.7+00.716 53 31-42 39 18H 1- 3342+00.1HARO 1952ESO 277-17, Sa 3- 38, VV' 146, Wray 16- 239 16.
PN G342.9-02.017 06 23-44 13 12Pe 1- 8342-02.117027-4409HENIZE 1964ESO 278-03, He 2- 198, Sa 2-173, VV' 159, Wray 16- 249 19. -1.0 ± 3.0 26.9 (O-III)
PN G343.0-01.717 05 39-43 57 27Vd 1-9343-01.117020-4352VANDERVORT 1964ESO 278-01 0.
PN G343.3-00.617 01 28-43 05 56HaTr 5HARTL et al 1983 120. B: 17.8, V: 16.4
PN G343.4+11.916 13 28-34 35 42H 1- 1343+11.1HARO 1952ESO 389-16, Sa 2-135, StWr 4- 5, VV' 134, Wray 16- 209 2.4 AG82 201, HARO 1- 1B: 16.87, V: 17.30
PN G343.6+03.716 44 24-40 03 20SuWt 3SCHUSTER et al 1980 20. -194.0 ± 15.0AG82 213B: 20.5, V: 20.5
PN G343.9+00.816 57 24-41 37 56H 1- 5344+00.116538-4133HARO 1952ESO 332-15, Sa 3- 39, VV' 149, Wray 16- 243 5.2
PN G344.2+04.716 42 33-38 54 27Vd 1-1344+04.116391-3848VANDERVORT 1964ESO 331-08, He 2- 178, Sa 2-151, Wray 16- 231 0. -142.1 ± 3.5B: 16.9, V: 16.7
PN G344.2-01.217 07 00-42 41 15H 1- 6344-01.1HARO 1952ESO 278-04, He 2- 199, Sa 3- 40, VV' 160, Wray 16- 250 12.
PN G344.4+02.816 50 33-40 03 00Vd 1-5344+02.1VANDERVORT 1964ESO 332-04, Sa 2-156 0.
PN G344.4-06.117 30 04-45 22 50Wray 16-278WRAY 1966Sa 2-208 0.
PN G344.8+03.416 49 33-39 21 10Vd 1-3344+03.1VANDERVORT 1964ESO 332-02, Sa 3- 37 0.
PN G345.0+03.416 50 25-39 08 19Vd 1-4345+03.116469-3903VANDERVORT 1964ESO 332-03, He 3-1261, Sa 2-154, Wray 16- 235 5. :
PN G345.0+04.316 46 45-38 36 58Vd 1-2345+04.116433-3831VANDERVORT 1964ESO 332-01 0.
PN G345.0-04.917 26 12-44 11 29Cn 1-3345-04.117225-4408CANNON 1921ESO 278-09, He 2- 220, PC 15, Sa 2-195, StWr 2-30, Wray 16- 272< 5. -78.0 ± 5.0B: 14.6, V: 14.3
PN G345.2-01.217 10 27-41 52 49H 1- 7345-01.117069-4149HARO 1952AS 219, ESO 332-24, He 2- 200, Sa 2-174, VV' 164, Wray 16- 254 8.5 AG82 231
PN G345.4+00.117 05 09-40 52 57IC 4637345+00.1FLEMING 1901ESO 332-21, He 2- 193, Sa 2-168, VV 89, VV' 156, Wray 15-1607 18.5 1.5 +11.2 ± 4.9 21.0 (O-III)AG82 224, CD -40 11127, CPD -40 7710, GCRV 9841, HD 154072B: 12.88, V: 12.50O(H)
PN G345.6+06.716 39 28-36 34 22He 2-175345+06.116361-3628HENIZE 1964ESO 391-01, Sa 2-150, Wray 16- 229 6.6 -32.0 ± 5.0
PN G345.9+03.016 54 27-38 44 08Vd 1-6345+03.216510-3839VANDERVORT 1964ESO 332-07, Sa 2- 159, Wray 16- 241 20. :
PN G346.0+08.516 34 04-35 05 26He 2-171346+08.116307-3459HENIZE 1964ESO 390-07, Wray 16- 226< 10. -83.0 ± 25.0
PN G346.2-08.217 45 29-44 54 11IC 4663346-08.117417-4453FLEMING 1901ESO 279-06, He 2- 273, Sa 2- 236, StWr 2- 32, VV 111, VV' 239, Wray 16- 303 13. -48.7 ± 9.0 15.0 (O-III)AG82 256, CSI -44 -17417, HD 161028B: 16.0, V: 15.2IUE obsns
PN G346.3-06.817 39 20-44 09 38Fg 2346-06.117356-4408FLEMING 1909ESO 279-04, He 2- 257, Sa 2-225, StWr 2-31, VV 106, VV' 224, Wray 16- 293< 5. +35.0 ± 4.0
PN G346.9+12.416 23 17-31 44 57K 1- 3346+12.1KOHOUTEK 1962A 38, ESO 452-01, Wray 19- 45 92. -12.8 ± 6.0 17.0 (O-III)AG82 207B: 20.5
PN G347.4+05.816 48 53-35 47 13H 1- 2347+05.116456-3542HARO 1952AS 208, ESO 391- 03, He 2- 181, MHa 300- 58, Sa 2-153, VV' 144, Wray 16- 234 0. 0.8 -102.0 ± 5.0
PN G347.7+02.017 04 34-37 53 13Vd 1-8347+01.117011-3749VANDERVORT 1964ESO 332-18, Sa 2- 167 0.
PN G348.0+06.316 48 48-35 00 57MGP 1MANCHADO et al 1989RPZM 2- 1, Wray 15-1537 3.8 B: 18.2
PN G348.4-04.117 32 48-40 58 24H 1-21348-04.117292-4056HARO 1952ESO 333-13, Sa 2-213, VV' 211, Wray 16- 284 0.
PN G348.8-09.017 56 33-43 03 17He 2-306348-09.117529-4302HENIZE 1964ESO 279-12, Sa 2-267, StWr 2-29, Wray 16- 330 3. B: 16.4, V: 16.8
PN G349.2-03.517 32 20-39 51 20H 2-14349-03.1HARO 1952ESO 333-11, Sa 3- 62, RPZM 2-22, VV' 210 20. : 15.
PN G349.3-01.117 22 16-38 28 58NGC 6337349-01.117188-3826HERSCHEL 1834ESO 333-05, H 1-10, He 2- 215, Sa 2- 191, Sh 1- 6, VV' 181, Wray 16- 267 51. -71.0 ± 4.0 7.8 (O-III)AG82 236B: 15.5, V: 14.90
PN G349.3-04.217 35 40-40 12 00Lo 1617322-4009LONGMORE 1977 83. AG82 248B: 17.3, V: 16.8
PN G349.5+01.017 13 44-37 06 06NGC 6302349+01.117103-3702FLEMING 1896ARO 502, ESO 392-05, Gum 60, He 2- 204, RCW 124, Sa 2- 180, Sh 1- 3, Sh 2- 6, VV 94, VV' 168, Wray 16- 259 44.5 10. -39.0 ± 2.1 8.0 (O-III)AG82 233, CD -36 11341, CPC 18 8579, GCRV 9926, HD 155520B: >21.1
PN G349.8+04.417 01 06-34 49 39M 2- 4349+04.116578-3445MINKOWSKI 1947ESO 391-07, He 2- 188, Sa 2-163, VV 84, VV' 150, Wray 16- 2456< 5. 2. -184.0 ± 11.0B: 17.6, V: 17.0
PN G350.1-03.917 36 30-39 22 02H 1-26350-03.117330-3920HARO 1952ESO 334-01, He 2- 253, Sa 2-220, VV' 220, Wray 16- 291 18. -37.0 ± 5.0
PN G350.5-05.017 42 54-39 36 28H 1-28350-05.117394-3935HARO 1952ESO 334-05, He 2- 268, Sa 2-231, VV4 233, Wray 15-1760 7.8 -45.0 ± 5.0
PN G350.8-02.417 32 20-37 57 38H 1-22350-02.117289-3755HARO 1952ESO 333-12, He 2- 241, Sa 2-212, VV' 212, Wray 16- 283 0. -213.0 ± 5.0
PN G350.9+04.417 04 37-33 59 12H 2- 1350+04.117013-3355HARO 1952MWC 247, ESO 392-02, He 2- 194, SaSt 2- 14, VV' 155, Wray 16- 247 5.6 2.2 4.6 -20.0 ± 5.5 13.0 (O-III)AG82 223B: 13.66, V: 13.26O(H)
PN G351.1+04.817 03 46-33 29 52M 1-19351+04.117005-3325MINKOWSKI 1946ESO 392-01, He 2- 191, Sa 2-165, VV' 153, Wray 15-1601 8. : 2.6 -40.0 ± 11.0B: 16.9
PN G351.2+05.217 02 19-33 10 04M 2- 5351+05.116590-3305MINKOWSKI 1947ESO 391-08, He 2- 190, SaSt 2-13, VV 86, VV' 152, Wray 16- 246 5. 5. -98.0 ± 11.0B: 16.4, V: 16.2
PN G351.3+07.616 53 37-31 40 35H 1- 4351+07.1HARO 1952ESO 453-09, Sa 2-158, VV' 147, Wray 16- 240 0. B: 16.3, V: 16.3
PN G351.6-06.217 50 44-39 17 24H 1-37351-06.117472-3916HARO 1952ESO 334-09, He 2- 291, Sa 2-251, VV' 262, Wray 16- 314 8.6 -16.0 ± 5.0
PN G351.9+09.016 50 17-30 19 55PC 13351+09.116471-3014PEIMBERT et al 1961ESO 453-06, Sa 2-155, StWr 4- 3, Wray 16- 236 7. : B: 16.7, V: 16.0
PN G351.9-01.917 33 00-36 43 53Wray 16-28617296-3641WRAY 1966ESO 393-06, Sa 2-215 0.
PN G352.0-04.617 45 07-38 08 49H 1-30352-04.117416-3807HARO 1952ESO 334-06, He 2- 272, VV' 237, Sa 2-23, Wray 16- 301 5.4 -8.0 ± 5.0
PN G352.1+05.117 05 31-32 32 09M 2- 8352+05.117022-3228MINKOWSKI 1947ESO 453-18, He 2- 197, Sa 2-170, VV 91, VV' 158, Wray 16- 248 4.2 3.7 +26.8 ± 11.8
PN G352.6+00.117 26 24-35 01 46H 1-12352+00.117230-3459HARO 1952ESO 392-12, He 2- 222, Sa 3- 51, VV' 190, Wray 16-273 6.8 11.
PN G352.6+03.017 14 43-33 24 48H 1- 8352+03.2HARO 1952ARO 549, ESO 392-06, Sa 2-182, VV' 170 3.4
PN G352.8-00.217 28 27-35 07 43H 1-13352-00.117251-3505HARO 1952ESO 393-01, He 2- 227, Sa 3-55, VV' 195, Wray 15-1712 9.6 14.
PN G352.9+11.416 44 49-28 04 05K 2-1616416-2758KOHOUTEK 1977ESO 453-02, Wray 17- 76, Anon 16h38 23. AG82 215B: 13.18, V: 12.75WC 11
PN G352.9-07.518 00 12-38 49 52Fg 3352-07.117567-3849FLEMING 1911ARO 520, ESO 334- 10, He 2- 320, Sa 2-277, StWr 2-26, VV 133, VV' 308, Wray 16- 346 2. +4.6 ± 2.0B: 14.3, V: 14.3
PN G353.2-05.217 50 45-37 23 54H 1-38353-05.1HARO 1952ESO 393-35, Sa 3- 81, VV' 264, Wray 16- 315 7.
PN G353.3+06.317 04 18-30 53 29M 2- 6353+06.217012-3049MINKOWSKI 1947ESO 453-16, He 2- 192, Sa 2-166, VV 88, VV' 154 8. : 1.6 -88.7 ± 14.4B: 16.67, V: 16.40
PN G353.5-04.917 49 48-37 01 27H 1-36353-04.117463-3700HARO 1952ESO 393-31, He 2- 289, Sa 2-249, VV' 259 0. -120.9 ± 3.1V: 16.8
PN G353.7+06.317 05 14-30 32 28M 2- 7353+06.117020-3028MINKOWSKI 1947ESO 453-17, He 2- 196, Sa 2-169, VV 90, VV' 157, Wray 15-1509 7.8 -56.0 ± 11.0B: 14.72, V: 13.96
PN G354.2+04.317 14 07-31 19 42M 2-10354+04.117108-3116MINKOWSKI 1947ESO 454-01, He 2- 205, VV 95, VV' 169, Wray 15-1647 4. 4. -75.0 ± 11.0
PN G354.5+03.317 18 52-31 39 06Th 3- 4354+03.117156-3135THE 1964ESO 454-07, Sa 3- 44 0.
PN G354.9+03.517 19 20-31 12 34Th 3- 6355+03.317161-3109THE 1964ESO 454-09, Sa 3- 45 0.
PN G355.1+02.317 24 26-31 43 18Th 3-11355+02.317212-3140THE 1964ESO 454-18, Sa 3- 47 0.
PN G355.1-02.917 45 32-34 33 56H 1-31355-02.417422-3432HARO 1952ESO 393-21, He 2- 276, Sa 2-238, VV' 240, Wray 16- 305< 5. 0.7 +86.0 ± 11.0
PN G355.2-02.517 44 14-34 17 28H 1-29355-02.217409-3416HARO 1952ESO 193-16, He 2- 270, Sa 2-233, VV' 235, Wray 16- 299 0. -18.0 ± 5.0WC
PN G355.4-02.417 44 20-34 06 41M 3-14355-02.117410-3405MINKOWSKI 1948ARO 552, ESO 393-19, He 2- 271, Sa 2-234, VV' 236, Wray 16- 300 7.2 2.8 -76.0 ± 11.0
PN G355.4-04.017 51 12-34 55 26Hf 2-1355-04.117478-3454HOFFLEIT 1953ESO 393-37, Pe 1-10, Sa 2-253, VV' 266, Wray 16-316 9.4 12.
PN G355.6-02.717 46 06-34 03 46H 1-32355-02.317427-3402HARO 1952ESO 393-23, He 2- 278, Sa 2-241, VV' 245, Wray 16- 307< 5. 1. -188.0 ± 5.0
PN G355.7-03.017 47 50-34 08 00H 1-33355-03.1HARO 1952ESO 393-26, He 2- 283, VV' 248 0. 2.7 -117.0 ± 5.0
PN G355.7-03.417 48 58-34 21 55H 2-23355-03.2HARO 1952ESO 393-27, He 3-1489, Sa 2-246, VV' 255 0. B: 18.4, V: 17.7
PN G355.7-03.517 49 14-34 22 53H 1-35355-03.317459-3421HARO 1952ESO 393-29, He 2- 288, My 103, Sa 2-247, VV' 257, Wray 16- 311 2. 1.1 +160.0 ± 11.0B: 15.7, V: 15.4
PN G355.9+02.717 24 40-30 51 53Th 3-10355+02.217214-3049THE 1964ESO 454-21, Sa 3- 48 0. 2.
PN G355.9+03.617 21 32-30 20 48H 1- 9355+03.217183-3017HARO 1952AS 226, ESO 454-14, He 2- 213, VV' 176, Wray 15-1689, MHa 76- 33, EM* AS 226, Sa 2- 190 7. : 0.7 -148.0 ± 11.2> 40.0 (O-III)B: 16.6, V: 15.8
PN G355.9-04.217 52 59-34 38 23M 1-30355-04.217496-3437MINKOWSKI 1946ESO 394-05, He 2- 295, Sa 2-259, VV 120, VV' 271, Wray 16- 322< 5. 3.5 -98.0 ± 11.0B: 16.6, V: 16.4WC ?
PN G356.1+02.717 25 19-30 40 44Th 3-13356+02.117221-3038THE 1964ESO 454-24 0. < 2.
PN G356.1-03.317 49 51-34 00 16H 2-26356-03.1HARO 1952ESO 393-32, Sa 3- 79, VV' 261, Wray 17- 99 4.5
PN G356.2-04.417 54 33-34 22 21Cn 2-1356-04.117512-3421CANNON 1922ESO 394-10, He 2- 303, Sa 2-263, VV 126, VV' 281, Wra y 16- 327 2.4 1.7 -271.0 ± 25.0
PN G356.5+01.517 30 59-31 01 08Th 3-55356+01.217277-3058THE 1964ESO 455-10, Sa 3- 58 0. < 9.
PN G356.5-02.317 46 45-33 08 35M 1-27356-02.217434-3307MINKOWSKI 1946ESO 393-24, He 2- 280, VV 113, VV' 246, Wray 16- 308 5.3 8. -16.5 8.5 (O-III)AG82 262, SS73 102B: 15.58, V: 14.54
PN G356.5-03.617 51 50-33 47 37H 2-27356-03.217485-3346HARO 1952ESO 394-02, Sa 3- 83, VV' 269 0.
PN G356.5-03.917 53 21-33 56 00H 1-39356-03.317500-3355HARO 1952ESO 394-07, He 2- 300, VV' 277, Wray 16- 323< 5. 1.7 -50.0 ± 11.0B: 16.8, V: 16.3
PN G356.7-04.817 57 19-34 09 49H 1-41356-04.217539-3409HARO 1952AS 256, ESO 394-13, He 2- 308, MHa 304- 10, Sa 2-269, VV' 293, Wray 16- 333 9.6 +76.0 ± 5.0B: 16.3, V: 16.2
PN G356.8-05.418 00 19-34 27 42H 2-35356-05.1HARO 1952ESO 394-17, Sa 3-109, VV' 311 10.8 -195.0 ± 5.0
PN G357.1+01.917 30 51-30 17 14Th 3-24357+02.7THE 1964ESO 455-09 0.
PN G357.1-04.717 58 15-33 47 39H 1-43357-04.317549-3347HARO 1952ESO 394-15, He 2- 313, VV' 297, Wray 16-335 2. 3. +76.0 ± 11.0B: 15.91, V: 15.42
PN G357.2+01.417 33 17-30 26 31Al 2-HALLEN 1979 0.
PN G357.2+02.017 31 07-30 10 37H 2-13357+02.6HARO 1952ESO 455-12, VV' 209, Sa 3- 59, Wray 17- 86 0.
PN G357.2-04.517 57 25-33 35 43H 1-42357-04.117541-3335HARO 1952ESO 394-14, He 2- 310, Sa 2- 270, VV' 294, Wray 16- 334 5.8 -79.0 ± 5.0B: 17.3
PN G357.4-03.217 52 34-32 45 52M 2-16357-03.217492-3245MINKOWSKI 1947ESO 394-04, He 2- 297, Sa 2- 256, VV 121, VV' 273, Wray 16- 320 5.4 2.2 +106.0 ± 11.0
PN G357.4-03.517 53 38-32 58 53M 2-18357-03.417503-3258MINKOWSKI 1947ESO 394-08, He 2- 301, Sa 2- 261, VV 124, VV' 278, Wray 16- 324< 5. 1.5 -3.0 ± 11.0B: 17.7, V: 17.3
PN G357.4-04.617 58 33-33 28 37M 2-22357-04.217552-3328MINKOWSKI 1947ESO 394-16, He 2- 316, Sa 2-273, VV 132, VV' 302, Wray 16- 341 5.2 5. -92.0 ± 11.0B: 17.3, V: 16.5
PN G357.6+01.017 35 44-30 21 29TrBr 4TERZAN et al 1978TeJu 21 30. -122. ± 60.
PN G357.6-03.317 53 17-32 40 41H 2-29357-03.317499-3240HARO 1952ESO 394-06, Sa 3- 87, VV' 276 4.8 AG82 268B: >21.
PN G357.9-03.817 56 14-32 37 34H 2-30358-03.217529-3236HARO 1952ESO 394-11, VV' 287 11.2 AG82 273B: >21.
PN G357.9-05.118 01 22-33 17 44M 1-34357-05.117580-3317MINKOWSKI 1946ESO 394-18, He 2- 324, Sa 2-279, VV 135, VV' 313, Wray 16- 348 11.2 +2.0 ± 11.0
PN G358.2-01.117 46 03-31 03 32Bl D358-01.1BLANCO 1961Al 2- L, ESO 455-34, Wray 17- 98 13.
PN G358.3-02.517 51 45-31 36 00Al 2-O17484-3135ALLEN 1979 2.4 -85.0
PN G358.5-02.517 52 10-31 30 03M 4- 7358-02.1MINKOWSKI 1948ESO 455-54, Al 2-P 7. 5.7
PN G358.5-04.217 59 02-32 21 44H 1-46358-04.117557-3221HARO 1952ESO 456-31, He 2- 318, Sa 2-274, VV' 306, Wray 16- 342 0. 1.2 -13.1 ± 10.1B: 16.8, V: 16.2
PN G358.7-02.717 53 37-31 25 33Al 2-RALLEN 1979 0.
PN G358.9-00.717 45 58-30 12 00M 1-26358-00.217427-3010MINKOWSKI 1946Bl C, AS 270, ESO 455-33, He 2- 277, RCW 135, SaSt 2-17, VV 112, VV' 242, Wray 16- 306 4.2 1.9 -5.0 ± 11.0 13.5 (O-III), 5.5 (N-II)AG82 260, HD 316248, MWC 270B: 13.44, V: 12.72Of(H)
PN G358.9-03.717 58 11-31 42 57H 1-44358-03.117549-3142HARO 1952ESO 456-23, He 2- 314, RCW 136, Sa 3-101, VV' 299, Wray 16- 336 3.6 +99.0 ± 5.0
PN G359.0-04.117 59 57-31 54 34M 3-48359-04.1MINKOWSKI 1948ESO 456-34, Sa 3-108, VV' 310, Wray 16- 345 4.9 -11.0 ± 5.0AG82 277B: >21.
PN G359.1-01.717 50 18-30 34 55M 1-29359-01.117471-3034MINKOWSKI 1946Bl F, ESO 455-47, He 2- 292, Sa 2-250, VV 119, VV' 263, Wray 16- 313 7.6 7. -62.0 ± 11.0
PN G359.1-02.317 52 47-30 49 45M 3-16359-02.217495-3048MINKOWSKI 1948VV' 272, Sa 2-258, ESO 456-02, Wray 16- 321, He 2- 296, Bl J=K 8.2 6.5 +81.0 ± 11.0B: 18.0, V: 17.2
PN G359.1-02.917 55 06-31 12 22M 3-46359-02.417518-3111MINKOWSKI 1948ESO 456-15, Sa 3- 93, VV' 283, Wray 17- 103 4.2 V: 17.9
PN G359.3-01.817 51 19-30 23 54M 3-44359-01.217480-3023MINKOWSKI 1948Bl H, ESO 455-51, Sa 3- 82, VV' 267, Wray 16- 317 4.4 4. -89.0 ± 11.0
PN G359.3-03.117 56 26-31 04 23M 3-17359-03.117531-3103MINKOWSKI 1948ESO 456-21, He 2- 307, Sa 3- 97, VV' 289, Wray 16- 331< 5. 2.9 -28.0 ± 11.0B: 18.1, V: 17.1
PN G359.4-03.417 58 13-31 08 08H 2-33359-03.217549-3107HARO 1952ESO 456-25, Sa 3-102, VV' 298, Wray 16- 338 6.2 AG82 275B: >21.
PN G359.7-01.817 52 05-30 05 18M 3-45359-01.317489-3004MINKOWSKI 1948Bl I, ESO 455-53, Sa 3- 84, VV' 270, Wray 17- 100 6.0 6.6 +32.0 ± 11.0
PN G359.7-02.617 55 36-30 33 32H 1-40359-02.317523-3033HARO 1952Bl 3-8, ARO 29, ESO 456-17, Sa 2-266, VV' 286, Wray 16- 328 3.8 1.3 +108.0 ± 11.0

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 [148]
IDNameRADecRSunRGCFe/HwtEB-VVHB(m-M)VVtMV,tU-BB-VV-RV-IsptellipvrvLSRsigvcrcrhμVρ0lg(tc)lg(th)
NGC 6093M 8016 17 02.41-22 58 33.910.03.8-1.7560.1816.1015.567.33-8.230.210.840.561.11F60.008.1 ± 1.516.712.4 ± 0.61.68 0.150.6115.114.797.788.80
NGC 6121M 416 23 35.22-26 31 32.72.25.9-1.16110.3513.4512.825.63-7.190.431.030.691.42F80.0070.7 ± 0.278.64.0 ± 0.21.65 1.164.3317.953.647.908.93
NGC 614416 27 13.86-26 01 24.68.92.7-1.7640.3616.4015.869.01-6.850.350.960.601.10F5/60.25193.8 ± 0.6201.91.55 0.941.6320.052.318.789.14
NGC 613916 27 40.37-38 50 55.510.13.6-1.6520.7517.9017.358.99-8.360.731.400.911.86F6/70.056.7 ± 6.011.51.86 0.150.8517.204.677.669.05
Terzan 316 28 40.08-35 21 12.58.22.5-0.7420.7317.5116.8212.00-4.82-136.3 ± 0.7-130.60.70 1.181.2522.521.828.798.57
1636-283ESO452-SC1116 39 25.45-28 23 55.38.32.1-1.5010.4616.6016.0212.00-4.021.00 0.500.5020.752.508.077.87
NGC 625616 59 32.62-37 07 17.010.33.0-1.0221.0919.0918.4411.29-7.151.031.69-101.4 ± 1.9-95.66.6 ± 2.62.50 c0.020.8617.895.595.828.86
Terzan 2HP 317 27 33.10-30 48 08.47.50.8-0.6931.8720.8720.1714.29-5.88109.0 ± 15.0116.92.50 c0.031.5222.164.865.468.82
Terzan 4HP 417 30 39.00-31 35 43.97.21.0-1.4142.0021.0720.4816.00-4.48-50.0 ± 2.9-42.30.90 0.901.858.70
Liller 117 33 24.50-33 23 20.48.20.8-0.3343.0724.8424.0916.77-7.3252.0 ± 15.059.22.30 0.0624.005.286.620.00
NGC 6380Ton 117 34 28.0-39 04 0910.93.3-0.7521.1719.5018.8111.31-7.502.01-3.6 ± 2.52.11.55 c:0.340.7419.893.738.408.86
Terzan 1HP 217 35 47.8-30 28 116.71.3-1.0331.9920.9620.3115.90-4.41114.0 ± 14.0122.02.50 c0.043.8225.093.854.999.12
Ton 2Pismis 2617 36 10.5-38 33 128.21.4-0.7011.2419.1018.4112.24-6.17-184.4 ± 2.2-178.61.30 0.541.3022.162.858.238.82
NGC 638817 36 17.23-44 44 07.89.93.1-0.5560.3716.8516.136.72-9.410.661.170.711.47G20.0180.1 ± 0.884.218.9 ± 0.81.75 0.120.5214.495.377.728.90
Djorg 117 47 28.3-33 03 5613.75.7-1.5111.5821.1520.5813.60-6.98-362.4 ± 3.6-355.01.50 0.501.5923.102.688.710.00
NGC 644117 50 13.06-37 03 05.211.63.9-0.4660.4717.5116.787.15-9.630.811.270.791.62G20.0216.5 ± 1.022.918.0 ± 0.21.74 0.130.5714.855.267.939.09
Terzan 6HP 517 50 46.38-31 16 31.46.81.3-0.5622.3522.1621.4413.85-7.59126.0 ± 15.0133.92.50 c0.050.4420.765.836.468.22
NGC 645317 50 51.70-34 35 57.011.63.7-1.5040.6417.8817.3010.08-7.220.681.310.992.00F80.09-83.7 ± 8.3-76.72.50 c0.050.4417.074.956.738.52
NGC 649617 59 03.68-44 15 57.411.34.2-0.4630.1516.4715.748.54-7.200.450.98G40.16-112.7 ± 5.7-108.40.70 0.951.0220.171.998.949.04

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