Sternbild Vela (Segel des Schiffes)

Eigenschaften
Vela, das Segel des großen Schiffes, liegt im Band der Milchstraße. Die Sterne kappa und delta Velorum bilden zusammen mit iota und epsilon Carinae ein großes Kreuz, das von Unkundigen oft mit dem Kreuz des Südens weiter westlich verwechselt wird und deshalb Falsches Kreuz heißt. Die Fläche des Sternbildes beträgt 500 Quadratgrad und das Zentrum kulminiert jeweils etwa am 11. Februar um Mitternacht. [9, 15]
Sterne mit Eigennamen:
- γ2 Vel: Suhail Al Muhlif, Al Suhail Al Muhlif, "Spectral Gem Of Southern Skies"
- λ Vel: Alsuhail, Al Suhail Al Wazn, Suhail

Mythologie und Geschichte
Die Sterne des Sternbilds Vela gehörten früher zum Sternbild Argo Navis und bilden heute ein Teil dessen, was Lacaille vom ürsprünglichen Sternbild übriggelassen hat. Die anderen Teile sind Carina, Puppis und Pyxis. Argo Navis war das Schiff vom thessalischen Helden Jason und seiner Besatzung, den Argonauten aus der griechischen Sage. Es half bei der Suche nach dem goldenen Vlies des Widders und konnte sprechen und weissagen.
Die hellsten Sterne der vier Teil-Sternbilder des Argo Navis besitzen immer noch eine durchgehende Bezeichnung mit griechischen Buchstaben, da Johann Bayer das Sternbild vor Nicolas Louis de Lacaille in seine Uranometria aufgenommen hatte. [6, 7, 10]
Kataloge
HR | B | F | DM | HD | SAO | FK5 | IR | M* | ADS | VarID | RA | Dec | vMag | spType | dMag | Sep ["] | Remarks |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
HR 3178 | CD-50 3138 | 67249 | 235730 | 2626 | 08 04 42.4 | -50 35 26 | 5.95 | G5II | |||||||||
HR 3179 | CD-46 3764 | 67341 | 219400 | 08 05 20.4 | -46 58 44 | 6.19 | B3Vnp | ||||||||||
HR 3187 | CD-44 4051 | 67582 | 219422 | 3905 | 08 06 40.4 | -45 15 59 | 5.05 | K3III | VAR:6.70 - 6.80p. | ||||||||
HR 3203 | CD-48 3516 | 68161 | 219493 | 08 09 09.6 | -48 41 04 | 5.70 | B8Ib-II | ||||||||||
HR 3204 | CD-43 3998 | 68217 | 219502 | 2634 | Var? | 08 09 35.9 | -44 07 22 | 5.21 | B2IV-V | ||||||||
HR 3206 | γ1 | CD-46 3846 | 68243 | 219501 | W | B | 3930 | 08 09 29.3 | -47 20 45 | 4.27 | B1IV | 2.3 | 41.2 | D:Component B of 5 stars within 2' of HR 3207.,G:Gamma Velorum group.,SB:1.482575d, K 45.0k/s, V0 +9.7k/s, asini 0.916. | |||
HR 3207 | γ2 | CD-46 3847 | 68273 | 219504 | 309 | W | A | Gam2 Vel | 08 09 32.0 | -47 20 12 | 1.78 | WC8+O9I v | 2.3 | 41.2 | D:See HR 3206. Mag. and colors blended with other companions. C = CoD -46d3848, 7.65V, B6V at 63", physical. D, 9.07V,,D:Am at 94", SB, over 7d?, optical.,G:Gamma Velorum group which includes HR 3206, probably also HD 68157 at 20' and HR 3213 at 36' from A; HII region.,M:Low degree of polarization indicates symmetric shell. The brightest O-type star and one of only four WR stars bright,M:enough to have been observed spectroscopically in UV by COPERNICUS. With 3165, appears capable of producing most of the,M:observed ionization of Gum Neb. The brightest and presumably the nearest Wolf-Rayet binary. Radio emission interpreted,M:as coming from circumstellar gas cloud extending farther than the orbital radius of the binary.,N:Suhail al Muhlif; Al Suhail al Muhlif; "Spectral Gem of Southern Skies".,R:Diam. = 0.00043 - 0.00044".,S:Magnesium and iron depleted by factor of 100 relative to the sun. UV spectrum dominated by supergiant companions. The,S:Wolf-Rayet component appears to be the most massive known. Radio emission indicates a circumstellar gas cloud extending,S:beyond the orbit of the binary. Also classified WC8+O7.5e.,SB:Comp. A of visual double, 78.5d, K 43.1k/s, V0 -18.0k/s, asini 45.8. Alternate orbit 78.5002d, K 70k/s,,SB:V0 +12k/s, msin3i 32, asini 67. Possible mass transfer from WR to O-type component.,VAR:1.6 - 1.8V, 154 sec. Sp. var. in about 200 sec. Variability too great to be explained by the 78.5d SB companion.,VAR:Possibly a third close companion: a collapsed star of less than 2 solar masses. | ||
HR 3213 | CD-47 3653 | 68324 | 219515 | IS Vel | 08 09 43.2 | -47 56 15 | 5.23 | B1IVe | RV:Amp. about 20k/s. Period probably same as for light curve.,VAR:BetaC, Amp. 0.018u, 0.108d. | ||||||||
HR 3227 | CD-48 3576 | 68657 | 219565 | 08 11 11.1 | -48 27 43 | 5.82 | B3V | ||||||||||
HR 3232 | CD-46 3902 | 68808 | 219587 | AH Vel | 08 12 00.0 | -46 38 39 | 5.76 | F7Ib-II | VAR:Cep 5.50 - 5.86V, 4.22717d. Per. and form of light curve vary. | ||||||||
HR 3234 | CD-45 3892 | 68895 | 219602 | W | 08 12 30.9 | -46 15 51 | 6.03 | B5V | 0.8 | 0.4 | |||||||
HR 3244 | CD-46 3929 | 69144 | 219629 | W | Var | 08 13 36.2 | -46 59 31 | 5.13 | B2.5IV | 3.9 | 35. | D:Companion K5V, RV +7k/s, optical.,VAR:Amp. 0.03b. | |||||
HR 3247 | CD-49 3430 | 69194 | 235819 | 3957 | 08 13 34.1 | -50 11 46 | 5.51 | M1III | G:Praesepe cluster. | ||||||||
HR 3250 | CD-45 3914 | 69302 | 219657 | W | 08 14 23.9 | -45 50 04 | 5.83 | B2IV-V | 1.5 | 0.4 | |||||||
HR 3256 | CD-50 3227 | 69596 | 235838 | 08 15 23.3 | -50 26 58 | 6.44 | K3-4III | ||||||||||
HR 3294 | CD-48 3734 | 70930 | 219848 | W | Var? | 08 22 31.6 | -48 29 25 | 4.82 | B1V | 1.0 | 0.8 | ||||||
HR 3300 | CD-51 2980 | 71043 | 235933 | 08 22 55.2 | -52 07 26 | 5.85 | A0V | ||||||||||
HR 3330 | CD-51 3004 | 71510 | 235962 | W | 08 25 31.0 | -51 43 41 | 5.17 | B2Ve | 4.2 | 25.7 | D:Component B, CoD-51d3003, 10.2v, B8V, optical. Third component G3V may be physical.,G:See HR 2702. | ||||||
HR 3341 | CP-52 1474 | 71722 | 235976 | 2661 | 08 26 25.2 | -52 48 27 | 6.05 | A0V | |||||||||
HR 3350 | CP-52 1484 | 71935 | 236002 | GU Vel | 08 27 36.5 | -53 05 19 | 5.09 | A9-F0III-IV | S:Also classified F3V.,VAR:Delta Sct amp. 0.015V, 0.07:d. | ||||||||
HR 3356 | CD-43 4337 | 72067 | 219982 | 2665 | W | 4106 | 08 29 07.6 | -44 09 38 | 5.79 | B2Vn t | 0.1 | 0.2 | VAR:H alpha emission var. | ||||
HR 3358 | CD-47 4004 | 72108 | 219985 | W | 08 29 04.7 | -47 55 45 | 5.33 | B2IV | 0.0 | 0.2 | D:AP, 6.4, 6.4v, sep. 0.176", combined mag., color. Components B, 7.7v at 4" binary with AP, C, 9.3v at 19".,SB:Comp. A of visual double; comp. B +15k/s. | ||||||
HR 3359 | CD-44 4462 | 72127 | 219996 | W | 08 29 27.6 | -44 43 30 | 4.99 | B2IV | 1.7 | 4.6 | D:Components B2III and B2.5V. | ||||||
HR 3363 | CD-45 4183 | 72232 | 220007 | 08 29 45.6 | -46 19 55 | 5.99 | B5III | ||||||||||
HR 3371 | CD-44 4477 | 72350 | 220025 | W | 08 30 39.2 | -44 44 14 | 6.30 | B4IV | 4.5 | 3.2 | G:Sco-Cen assoc. | ||||||
HR 3373 | CD-38 4566 | 72436 | 199329 | W | 08 31 24.6 | -39 03 51 | 6.31 | B4V | 1.8 | 3.8 | |||||||
HR 3375 | CD-47 4048 | 72485 | 220039 | 08 31 10.8 | -47 52 00 | 6.39 | B2.5V | ||||||||||
HR 3382 | CP-53 1729 | 72650 | 236055 | 08 31 29.6 | -54 23 39 | 6.34 | K3III | ||||||||||
HR 3386 | CP-52 1517 | 72737 | 236062 | W | 08 32 04.8 | -53 12 44 | 5.69 | K0III+A3 | 1.0 | 0.8 | D:SKYLAB indicates cool star with hot companion.,S:Also classified G8III + A0/1V. | ||||||
HR 3388 | CD-37 4850 | 72787 | 199363 | Var? | 08 33 19.9 | -38 22 16 | 6.49 | B2.5V | M:Old disk population runaway star. | ||||||||
HR 3389 | CD-38 4610 | 72832 | 199370 | 4137 | 08 33 38.3 | -38 50 56 | 5.96 | B5III | VAR:5.8 - 5.89B. | ||||||||
HR 3390 | CD-46 4300 | 72900 | 220103 | 08 33 30.4 | -46 58 16 | 6.24 | K3III | ||||||||||
HR 3399 | CD-37 4873 | 72993 | 199389 | W | 4143 | 08 34 29.3 | -37 36 41 | 6.30 | K5III | 2.3 | 1.9 | D:Components M1IIIa and G7IIIb.,VAR:Amp. 0.09V. | |||||
HR 3404 | CD-39 4519 | 73121 | 199402 | 08 35 12.6 | -39 58 12 | 6.47 | G1V | ||||||||||
HR 3407 | CD-49 3646 | 73155 | 220138 | 2674 | 08 34 43.6 | -49 56 39 | 5.01 | K1-2II | |||||||||
HR 3413 | CD-50 3417 | 73340 | 236110 | HV Vel | 08 35 52.1 | -50 58 12 | 5.80 | B8Si v | G:In cluster IC 2391.,VAR:Amp. 0.025y, 2.67d. Spectrum var. same period. | ||||||||
HR 3421 | CD-39 4574 | 73524 | 199438 | 08 37 19.9 | -40 08 51 | 6.55 | G4IV-V | ||||||||||
HR 3426 | CD-42 4451 | 73634 | 220204 | 324 | 08 37 38.7 | -42 59 21 | 4.14 | A6II | |||||||||
HR 3435 | CP-52 1565 | 73952 | 236142 | W | 08 38 44.9 | -53 05 26 | 6.47 | B8Vn | 7.5 | 22.2 | G:IC 2391 #8. | ||||||
HR 3439 | CD-39 4653 | 74067 | 220252 | W | 4193 | 08 40 19.3 | -40 15 51 | 5.20 | B9V | 3.7 | 4.4 | D:Companion A2V. | |||||
HR 3440 | CP-53 1796 | 74071 | 236151 | HW Vel | 08 39 23.8 | -53 26 23 | 5.48 | B5V | G:See HR 2702.,G:IC 2391 #13, probable member of the cluster.,VAR:Amp. 0.02V, 0.26145d. Probable beat phenomena. | ||||||||
HR 3442 | CP-52 1579 | 74146 | 236157 | W | 4194 | 08 39 57.6 | -53 03 18 | 5.19 | B4IV | 4.4 | 16.6 | D:CPM? Companion F0IV.,G:Sco-Cen assoc.; probable member of open cluster IC 2391 (#16). See HR 2702.,SB:Primary of visual double. 3.1d. RV comp. B +12k/s.,VAR:Component A of double. Ell?, 5.17 - 5.27V. | |||||
HR 3444 | CD-44 4679 | 74167 | 220261 | 4198 | 08 40 35.3 | -45 11 29 | 5.71 | M0III | |||||||||
HR 3445 | CD-46 4438 | 74180 | 220265 | 1226 | W | 4199 | 08 40 37.6 | -46 38 56 | 3.84 | F3Ia | 6.9 | 37.5 | C:U-B values scatter from +0.22 to +0.54.,G:Vel OB1. | ||||
HR 3447 | CP-52 1583 | 74195 | 236164 | 1227 | o Vel | 08 40 17.6 | -52 55 19 | 3.62 | B3IV | G:In cluster IC 2391 #20.,N:Sometimes called omicron Vel, but the letter had originally been "o" (Roman), not omicron.,RV:Expanding circumstellar shell.,SB:3.2 hrs.,VAR:Beta C 3.56 - 3.67V, 0.131977d. | |||||||
HR 3448 | CP-52 1584 | 74196 | 236165 | 4197 | 08 40 17.4 | -53 00 55 | 5.61 | B7Vn | G:IC 2391 #21.,S:Helium-weak star.,VAR:Beta C?, 5.56 - 5.62V, amp. 0.01b, 0.388d. Possibly the shortest period known for a He-weak star. | ||||||||
HR 3452 | CD-46 4448 | 74272 | 220284 | 08 41 13.1 | -47 19 01 | 4.77 | A5II | ||||||||||
HR 3453 | CD-48 4020 | 74273 | 220282 | 08 41 05.3 | -48 55 21 | 5.90 | B1.5V | S:Also classified B2III. | |||||||||
HR 3456 | CD-44 4704 | 74371 | 220300 | 08 41 56.9 | -45 24 39 | 5.23 | B6Iae | G:Vel OB1. | |||||||||
HR 3462 | CD-47 4251 | 74455 | 220313 | W | HX Vel | 08 42 16.0 | -48 05 57 | 5.51 | B1.5Vn | 1.3 | 0.3 | G:In cluster IC 2395 #1; Sco-Cen assoc.,M:Unusually high-velocity interstellar CaII not associated with galactic rotation, but probably part of Vela supernova,M:remnant associated with Pulsar 0833-45 about 3d away.,VAR:Amp. 0.037b, 0.563d. | |||||
HR 3466 | CP-52 1605 | 74535 | 236202 | W | BC | KT Vel | 08 42 18.9 | -53 06 00 | 5.52 | B8Si | 0.8 | 76.6 | D:Binary with HR 3467. Component C 8.0v at 0.5" from B.,G:IC 2391 #31.,VAR:Alpha CV, 5.49 - 5.56V, 3.376d. | ||||
HR 3467 | CP-52 1607 | 74560 | 236205 | W | A | HY Vel | 08 42 25.5 | -53 06 50 | 4.86 | B3IV | 0.8 | 76.6 | D:See HR 3466.,G:Sco-Cen assoc.; IC 2391 #34, probable member of cluster. See HR 2702.,VAR:Amp. 0.015b, 0.0284d. | ||||
HR 3476 | CD-49 3761 | 74753 | 220361 | 2689 | 08 43 40.3 | -49 49 22 | 5.16 | B0IIIn | |||||||||
HR 3477 | CD-42 4569 | 74772 | 220371 | W | 08 44 24.0 | -42 38 57 | 4.07 | G5III | 7.1 | 45.3 | G:Possibly member open cluster Trumpler 10. | ||||||
HR 3485 | δ | CP-54 1788 | 74956 | 236232 | W | 08 44 42.2 | -54 42 30 | 1.96 | A1V | 3.0 | 2.2 | D:AB binary with CPM double companion CD at 69". CD 11.0, 13.5v sep. 6".,DYN:0.034".,G:In Ursa cluster? Sirius group?,RV:Two determinations of vsini, 0 and 80k/s. | |||||
HR 3487 | CD-45 4517 | 75063 | 220422 | 08 46 01.7 | -46 02 30 | 3.91 | A1III | ||||||||||
HR 3488 | CD-40 4602 | 75081 | 220432 | 08 46 23.8 | -41 07 32 | 6.21 | B9Ve t | VAR:H alpha emission var. | |||||||||
HR 3494 | CD-45 4526 | 75149 | 220442 | 08 46 30.6 | -45 54 46 | 5.46 | B3Ia | D:Wide CPM pair with HR 3496.,G:Sco-Cen assoc.; Vel OB1. | |||||||||
HR 3496 | CD-45 4541 | 75276 | 220464 | 08 47 18.9 | -46 09 20 | 5.75 | F2Iab | C:U-B values scatter from +0.22 to +0.55.,D:See HR 3494.,G:Vel OB1. | |||||||||
HR 3497 | CD-41 4507 | 75289 | 220481 | 08 47 40.5 | -41 44 14 | 6.36 | G0Ia-0: | ||||||||||
HR 3501 | CD-41 4516 | 75387 | 220495 | 08 48 08.8 | -42 27 50 | 6.43 | B2IV-V | G:In open cluster Trumpler 10. | |||||||||
HR 3503 | CP-52 1675 | 75466 | 236284 | 08 48 00.2 | -52 51 02 | 6.30 | B8V | G:IC 2391 #50.,RV:Other determinations as high as +34k/s. | |||||||||
HR 3514 | CD-39 4838 | 75630 | 220531 | 08 49 39.2 | -40 19 14 | 5.48 | A2/3IV | ||||||||||
HR 3517 | CD-38 4925 | 75654 | 199682 | 2697 | HZ Vel | 08 49 52.4 | -39 08 30 | 6.39 | A5III | VAR:Delta Sct, 0.087d. | |||||||
HR 3520 | CD-44 4861 | 75710 | 220540 | 2698 | 08 49 47.7 | -45 18 29 | 4.93 | A2III | |||||||||
HR 3525 | CD-41 4560 | 75759 | 220552 | 08 50 21.0 | -42 05 24 | 6.00 | B1-2III | G:Sco-Cen assoc.; doubtful member Vel OB1.,S:Also classified O9IV, O9V, B0V, B1IIIn.,SB:33.311d, K 121.3k/s, V0 +23.4k/s, msin3i 18.0, a1sini 43.1, a2sini 53.5. Massive system similar to,SB:Iota Ori; might be eclipsing. | |||||||||
HR 3527 | CD-46 4661 | 75821 | 220561 | W | 08 50 33.5 | -46 31 45 | 5.10 | B0III | 4.1 | 3.2 | D:CPM.,G:Sco-Cen assoc.,RV:High-velocity interstellar CaII not associated with galactic rotation, but probably part of Vela SN remnant associated,RV:with Pulsar 0833-45 about 3d away. | ||||||
HR 3530 | CD-42 4723 | 75926 | 220581 | 08 51 27.9 | -42 30 16 | 6.55 | A1Vn | ||||||||||
HR 3535 | CD-38 4980 | 76110 | 199737 | 08 52 48.0 | -38 43 27 | 5.82 | M0III | ||||||||||
HR 3539 | CD-47 4460 | 76161 | 220609 | 08 52 38.6 | -48 21 33 | 5.91 | B3Vn | G:Sco-Cen assoc. | |||||||||
HR 3542 | CD-51 3303 | 76230 | 236362 | W | 08 52 40.8 | -52 07 45 | 6.39 | A0V | 1.6 | 2.8 | D:Binary. Combined mag., colors. | ||||||
HR 3548 | CD-39 4924 | 76304 | 220628 | 08 53 50.7 | -40 26 51 | 6.47 | K0II-III+A5 | ||||||||||
HR 3551 | CD-47 4480 | 76360 | 220636 | W | 08 53 50.7 | -47 31 15 | 5.33 | A9IV-V | 0.0 | 0.1 | D:6.1 Am, 6.1, 7.24y, a = 0.1036". Combined mag., color.,DYN:0.017".,SB:9.07d. | ||||||
HR 3562 | CD-44 4951 | 76566 | 220664 | W | IY Vel | 08 55 19.3 | -45 02 30 | 6.26 | B3IV | 6.5 | 35.0 | VAR:Amp. 0.04:V. Multiple periods 1.97, 1.73 and 1.66d found, but subsequently questioned. | |||||
HR 3570 | CP-54 1925 | 76653 | 236405 | 08 55 11.9 | -54 57 56 | 5.71 | F6V | ||||||||||
HR 3574 | CP-52 1788 | 76805 | 236417 | W | 08 56 19.4 | -52 43 25 | 4.69 | B5V | 3.0 | 2.8 | SB:0.9147d, K 46.3k/s, V0 +22.2k/s, asini 0.577. | ||||||
HR 3583 | CD-48 4282 | 77020 | 220703 | 08 57 55.8 | -48 34 24 | 5.87 | G8-K0II | ||||||||||
HR 3588 | CD-46 4810 | 77140 | 220717 | W | FZ Vel | 08 58 52.3 | -47 14 05 | 5.18 | Am | 6.0 | 24.2 | G:Hyades moving group.,S:Delta Sct type spectrum.,VAR:Delta Sct 5.15 - 5.17V, 0.065d. | |||||
HR 3591 | CD-40 4810 | 77258 | 220730 | 1234 | 4346 | 09 00 05.4 | -41 15 14 | 4.45 | G8-K1III+A | S:Also variously classified Fp, F8III.,SB:74.1469d, K 17.8k/s, V0 -7.4k/s, asini 18.1. | |||||||
HR 3593 | CD-42 4875 | 77320 | 220738 | IU Vel | 09 00 22.2 | -43 10 24 | 6.07 | B2.5Vn t | S:Variable H alpha emission.,VAR:Beta Cep 6.02 - 6.06V, about 7 hrs. with beat phenomenon. | ||||||||
HR 3600 | CD-41 4720 | 77475 | 220760 | IZ Vel | 09 01 20.8 | -41 51 52 | 5.55 | B5V | VAR:Amp. 0.03:V. Multiple periods 9.64, 14.4 and 10.7d. | ||||||||
HR 3602 | CD-38 5154 | 77580 | 199902 | 09 02 06.4 | -39 24 09 | 6.27 | K1III-IV | ||||||||||
HR 3605 | CD-51 3430 | 77653 | 236518 | W | 09 01 44.6 | -52 11 18 | 5.23 | B9Si | 1.2 | 0.9 | |||||||
HR 3611 | CP-53 2072 | 77907 | 236542 | 09 03 05.2 | -53 32 59 | 6.40 | B6V | ||||||||||
HR 3614 | CD-46 4883 | 78004 | 220803 | 342 | 09 04 09.3 | -47 05 52 | 3.75 | K2III | |||||||||
HR 3629 | CP-55 1957 | 78548 | 236611 | 09 06 34.0 | -55 48 12 | 6.11 | B2IV-V | ||||||||||
HR 3631 | CD-50 3849 | 78599 | 236618 | 2722 | 09 07 14.7 | -51 12 43 | 6.73 | K4III | |||||||||
HR 3634 | λ | CD-42 4990 | 78647 | 220878 | 345 | I | W | Lam Vel | 09 07 59.8 | -43 25 57 | 2.21 | K4.5Ib-II e | 12.6 | 18.2 | M:Young disk population.,N:Alsuhail; Al Suhail al Wazn; Suhail.,S:Ultraviolet FeII emission.,VAR:Lc 2.14 - 2.22V. | ||
HR 3647 | CD-48 4471 | 79025 | 220910 | 09 09 45.1 | -49 25 29 | 6.48 | A9Vn | S:Also classified Am. | |||||||||
HR 3654 | CD-44 5206 | 79186 | 220928 | GX Vel | 09 11 04.4 | -44 52 05 | 5.00 | B5Ia | VAR:Amp. 0.07V. | ||||||||
HR 3656 | CD-38 5358 | 79241 | 200084 | 09 11 41.0 | -39 15 32 | 6.00 | B6V | ||||||||||
HR 3658 | CD-46 4987 | 79275 | 220937 | 09 11 33.2 | -46 35 02 | 5.79 | B2III/IV | ||||||||||
HR 3661 | CD-43 5041 | 79416 | 220952 | W | KL Vel | 09 12 30.6 | -43 36 49 | 5.57 | B8Vp:Si: | 0.7 | 2.8 | D:AB 6.7, 7.2v sep. 0.11". Combined mag., colors of ABC. | |||||
HR 3667 | CD-38 5376 | 79523 | 200119 | 4423 | 09 13 25.9 | -38 36 59 | 6.31 | A0V | |||||||||
HR 3668 | CD-41 4904 | 79524 | 220962 | 09 13 18.6 | -42 16 25 | 6.29 | K2III | ||||||||||
HR 3670 | CD-46 5010 | 79621 | 220965 | 09 13 34.5 | -47 20 19 | 5.92 | B9Ve v | S:Variable H alpha. | |||||||||
HR 3672 | CD-43 5068 | 79694 | 220972 | 2731 | 4428 | 09 14 08.2 | -44 08 45 | 5.85 | B5/6IV/V | G:Sco-Cen assoc. See HR 2702. | |||||||
HR 3674 | CD-42 5086 | 79735 | 220978 | W | 09 14 24.5 | -43 13 39 | 5.25 | B4V | 4.1 | 5.8 | G:Sco-Cen assoc. See HR 2702. | ||||||
HR 3677 | CD-37 5578 | 79807 | 200152 | 09 14 57.2 | -37 36 09 | 5.86 | G0V | ||||||||||
HR 3679 | CP-55 2035 | 79846 | 236749 | 2736 | 4429 | 09 14 18.0 | -55 34 11 | 5.27 | G8II-III | VAR:6.3 - 8.1p. | |||||||
HR 3680 | CD-45 4982 | 79900 | 220998 | W | 09 15 14.6 | -45 33 20 | 6.25 | B8V | 0.9 | 0.8 | D:Binary, combined mag., colors. | ||||||
HR 3682 | CD-38 5408 | 79917 | 200159 | 2737 | 09 15 36.7 | -38 34 12 | 4.94 | K0III | |||||||||
HR 3684 | CD-36 5505 | 79940 | 200163 | W | 09 15 45.1 | -37 24 48 | 4.62 | F5III | 9.8 | 11.3 | |||||||
HR 3688 | CD-44 5305 | 80057 | 221010 | W | 4436 | 09 16 04.2 | -44 53 55 | 6.04 | A1Ib | 8.0 | 6.8 | VAR:6.3 - 6.34p. | |||||
HR 3692 | CD-43 5103 | 80108 | 221014 | 4437 | 09 16 23.1 | -44 15 57 | 5.12 | K3Ib | S:Also classified K4III.,VAR:5.08 - 5.14V. | ||||||||
HR 3694 | CD-38 5430 | 80170 | 200185 | 09 16 57.2 | -39 24 05 | 5.33 | K5III-IV | RV:Period 1 - 2 months? | |||||||||
HR 3700 | CP-53 2281 | 80435 | 236819 | 09 17 42.3 | -54 29 43 | 6.33 | K3III | ||||||||||
HR 3703 | CD-50 4001 | 80456 | 236824 | 09 18 05.8 | -51 03 04 | 5.26 | B7-8III | ||||||||||
HR 3708 | CD-51 3693 | 80558 | 236837 | 4454 | 09 18 42.2 | -51 33 38 | 5.87 | B6Iae | C:B-V values scatter from +0.43 to +0.62, U-B from -0.16 to -0.40. | ||||||||
HR 3716 | CD-37 5668 | 80774 | 200257 | 09 20 29.6 | -37 34 53 | 6.05 | K3/4III | ||||||||||
HR 3717 | CP-54 2186 | 80781 | 236851 | 09 19 32.6 | -55 11 12 | 6.28 | B5V | G:Formerly considered member of Sco-Cen assoc. (probably not member).,M:Close to error box of X-ray source 3U0918-55. | |||||||||
HR 3726 | CD-41 5023 | 81034 | 221103 | 09 21 50.9 | -42 11 42 | 5.58 | M1III | ||||||||||
HR 3729 | CD-39 5446 | 81134 | 200299 | 09 22 36.7 | -39 46 29 | 6.54 | K1III | ||||||||||
HR 3730 | CD-45 5099 | 81136 | 221109 | 2746 | 4473 | 09 22 24.0 | -46 02 51 | 5.75 | G6-8III | VAR:5.72 - 5.76V. | |||||||
HR 3732 | CP-54 2213 | 81157 | 236887 | 09 21 50.0 | -55 30 54 | 5.63 | A3IV s: | ||||||||||
HR 3734 | κ | CP-54 2219 | 81188 | 236891 | 353 | 09 22 06.8 | -55 00 39 | 2.50 | B2IV-V | G:Sco-Cen assoc.,M:Third UHURU Catalogue suggests Kappa Vel as optical counterpart of 3U0918-55, but HR 3717 is much closer.,SB:116.65d, K 46.5k/s, V0 +21.9k/s, asini 73.2. | |||||||
HR 3735 | CD-37 5721 | 81309 | 200320 | 09 23 44.8 | -37 45 26 | 6.48 | A1mA5-F0 | ||||||||||
HR 3737 | CD-38 5541 | 81411 | 200330 | W | 09 24 16.3 | -39 25 33 | 6.06 | A7V: | 0.0 | 0.1 | S:Also classified A6/7III. | ||||||
HR 3739 | CD-51 3767 | 81471 | 236930 | 09 23 59.5 | -51 44 14 | 6.08 | A7Iab | C:B-V values scatter from +0.49 to +0.66, U-B from +0.06 to +0.39. | |||||||||
HR 3746 | CD-39 5507 | 81780 | 221167 | 09 26 28.5 | -40 30 07 | 6.20 | A7III | ||||||||||
HR 3753 | CP-52 2360 | 81848 | 236972 | 09 26 18.1 | -53 22 45 | 5.11 | B6V | G:Sco-Cen assoc. | |||||||||
HR 3784 | CD-50 4204 | 82419 | 237042 | 09 30 05.2 | -51 31 02 | 5.45 | B8V | ||||||||||
HR 3786 | ψ | CD-39 5580 | 82434 | 221234 | W | 4513 | 09 30 42.0 | -40 28 00 | 3.60 | F3IV+F0IV | 0.5 | 0.7 | D:4.1 F2IV, 4.6 F0V, 33.99y, a = 0.795". Combined mag., colors.,DYN:0.061".,VAR:Comp. B, 4.5 - 5.1v. | ||||
HR 3803 | CP-56 2270 | 82668 | 237067 | 361 | N Vel | 09 31 13.3 | -57 02 04 | 3.13 | K5III | VAR:L? 3.10 - 3.16V. | |||||||
HR 3807 | CD-40 5284 | 82694 | 221262 | 2759 | W | 09 32 19.3 | -40 38 58 | 5.35 | G8III | 3.6 | 1.1 | ||||||
HR 3817 | CD-48 4802 | 82984 | 221288 | W | 09 33 44.5 | -49 00 18 | 5.12 | B4IV | 0.8 | 2.1 | D:Secondary B8V, vsini 157k/s.,G:Sco-Cen assoc.; probable member of Sco-Cen cluster.,RV:Comp. A of double, RV var.; comp. B +20k/s. | ||||||
HR 3819 | CD-50 4270 | 83058 | 237107 | 2764 | 09 34 08.8 | -51 15 19 | 5.01 | B1.5IV | |||||||||
HR 3831 | CD-48 4831 | 83368 | 221339 | W | IM Vel | 09 36 25.3 | -48 45 05 | 6.17 | ApSrEuCr | 2.4 | 3.1 | RV:Detailed analysis by Kurtz and Marang (1988, MNRAS, 231, 1039) gives rotational frequency of 4.05829 microHz (2.85196d).,S:Also classified A7pSr.,VAR:Amp. 0.05V, 2.8519d. Also pulsations of 11.67 min. | |||||
HR 3836 | CD-48 4836 | 83446 | 221344 | 2768 | W | 09 36 49.6 | -49 21 19 | 4.35 | A5IV-V | 8.7 | 25.7 | ||||||
HR 3837 | CP-52 2612 | 83465 | 237144 | 09 36 46.3 | -52 56 39 | 6.19 | K0III | ||||||||||
HR 3840 | CP-53 2646 | 83520 | 237149 | W | 09 37 12.3 | -53 40 07 | 5.45 | A2-3V | 0.0 | 0.5 | D:CPM. | ||||||
HR 3842 | CD-42 5462 | 83548 | 221355 | 2771 | 09 38 01.5 | -43 11 28 | 5.50 | G8II | S:BaII star. Overabundance of praseodymium. | ||||||||
HR 3868 | CP-54 2594 | 84228 | 237237 | 09 41 47.8 | -55 12 51 | 6.00 | B4V | ||||||||||
HR 3872 | CD-50 4420 | 84400 | 237260 | W | IP Vel | 09 43 27.5 | -51 13 42 | 6.15 | B6V | 4.7 | 2.1 | VAR:E amp. 0.2b. Component A of visual double. | |||||
HR 3875 | CP-53 2788 | 84461 | 237268 | 09 43 42.2 | -53 53 30 | 5.56 | A0IV | G:Sco-Cen assoc. | |||||||||
HR 3886 | CD-44 5846 | 84816 | 221484 | Var? | 09 46 30.4 | -44 45 18 | 5.55 | B2.5IV | G:Sco-Cen assoc. | ||||||||
HR 3895 | CP-55 2548 | 85250 | 237370 | 09 48 40.0 | -56 24 43 | 6.06 | K0III | G:NGC 3033 #1. | |||||||||
HR 3898 | CD-45 5470 | 85355 | 221523 | W | 09 49 57.1 | -45 43 58 | 5.08 | B7III | 4.5 | 66.6 | D:Secondary B9. | ||||||
HR 3904 | CD-46 5558 | 85483 | 221538 | 09 50 42.0 | -46 56 04 | 5.73 | K0IIICNIb | ||||||||||
HR 3910 | CD-45 5499 | 85563 | 221547 | 1256 | 09 51 19.8 | -46 11 38 | 5.62 | K2III | |||||||||
HR 3912 | CD-45 5508 | 85622 | 221553 | 4658 | 09 51 40.8 | -46 32 52 | 4.58 | G5Ib | SB:329.30d, K 14.1k/s, V0 +11.0k/s, asini 63.8. | ||||||||
HR 3920 | CP-54 2816 | 85871 | 237448 | 4668 | 09 53 00.0 | -55 22 24 | 6.48 | B1IV | VAR:6.3 - 6.36B. | ||||||||
HR 3924 | CD-50 4622 | 85953 | 237464 | Var? | 09 53 50.2 | -51 08 49 | 5.93 | B2III | VAR:BetaC, Amp. 0.03b, 0.1096d. | ||||||||
HR 3925 | CD-44 5987 | 85980 | 221592 | W | 09 54 17.6 | -45 17 02 | 5.71 | B3V | 2.4 | 5.3 | D:Binary. Combined mag., colors.,G:Sco-Cen cluster.,RV:Component B, +5k/s. | ||||||
HR 3927 | CD-49 4801 | 86087 | 237483 | 09 54 51.3 | -50 14 38 | 5.72 | A0V | SB:Equal components. | |||||||||
HR 3930 | CD-40 5626 | 86211 | 221617 | 2795 | 09 56 05.4 | -40 49 29 | 6.41 | M1III | |||||||||
HR 3935 | CD-50 4662 | 86352 | 237514 | 2797 | 09 56 21.9 | -51 20 10 | 6.37 | B2IV-V | |||||||||
HR 3940 | φ | CP-53 3075 | 86440 | 237522 | 375 | W | 09 56 51.8 | -54 34 04 | 3.54 | B5Ib | 8.3 | 37.2 | D:Companion K0III, optical.,G:Sco-Cen assoc. | ||||
HR 3941 | CP-52 2980 | 86466 | 237526 | IV Vel | 09 57 10.9 | -52 38 20 | 6.12 | B3IV | G:Sco-Cen assoc.; probable member of Sco-Cen cluster.,VAR:BetaC, amp. 0.013b, 0.1608d. | ||||||||
HR 3943 | CD-47 5399 | 86523 | 221644 | W | 09 57 42.5 | -48 24 52 | 6.05 | B3V | 4.6 | 14.1 | D:CPM companion A0III; however, the companion is optical. | ||||||
HR 3953 | CP-56 2746 | 87030 | 237586 | W | 10 00 34.4 | -56 56 48 | 6.52 | K0III | 6.5 | 7.6 | |||||||
HR 3955 | CP-52 3087 | 87152 | 237612 | Var? | 10 01 40.5 | -53 21 52 | 6.20 | B2.5V | G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster. | ||||||||
HR 3964 | CD-46 5759 | 87363 | 221728 | 10 03 20.5 | -46 38 10 | 6.12 | A0V | ||||||||||
HR 3976 | CD-46 5806 | 87783 | 221773 | W | 10 06 11.3 | -47 22 12 | 5.08 | K1IV+G5V | 1.7 | 0.7 | D:5.3 K0IV, 6.9 G5V, 232y, a = 0.64". Combined mag., colors. | ||||||
HR 3978 | CD-51 4471 | 87816 | 237690 | R Vel | 10 06 07.1 | -52 11 17 | 6.52 | K1III | VAR:Cst 6.49V. | ||||||||
HR 3990 | CD-51 4507 | 88206 | 237736 | 10 08 56.3 | -51 48 40 | 4.86 | B3IV | G:Sco-Cen assoc. | |||||||||
HR 4001 | CD-41 5658 | 88399 | 221832 | 10 10 37.9 | -41 42 54 | 5.98 | K2-3III | ||||||||||
HR 4010 | CD-51 4560 | 88693 | 237784 | 10 12 23.0 | -52 09 48 | 6.16 | K2IIICNII | ||||||||||
HR 4017 | CD-50 4924 | 88824 | 237804 | 10 13 22.8 | -51 14 00 | 5.28 | A7V | ||||||||||
HR 4020 | CD-51 4578 | 88842 | 237807 | W | 4788 | 10 13 28.0 | -51 45 22 | 5.78 | A3IV-V | 1.5 | 0.3 | ||||||
HR 4023 | CD-41 5713 | 88955 | 221895 | 382 | I | 10 14 44.2 | -42 07 19 | 3.85 | A2V | G:Sco-Cen assoc. | |||||||
HR 4036 | CD-42 6074 | 89062 | 221910 | 10 15 31.5 | -43 06 45 | 5.60 | K4III | ||||||||||
HR 4038 | CP-54 3356 | 89104 | 237834 | Var? | 10 15 16.6 | -54 58 27 | 6.16 | B2IV-V | G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster. | ||||||||
HR 4045 | CD-50 4990 | 89273 | 237858 | GY Vel | 10 16 40.2 | -51 12 18 | 6.30 | M4-5III | VAR:Amp. 0.32V, 0.11R. | ||||||||
HR 4056 | CD-41 5765 | 89461 | 221948 | 10 18 28.2 | -41 40 06 | 5.96 | B9V | ||||||||||
HR 4061 | CP-55 3220 | 89569 | 237902 | 10 18 37.6 | -56 06 36 | 5.81 | F6V | ||||||||||
HR 4063 | CP-54 3474 | 89682 | 237916 | 2830 | GZ Vel | 10 19 36.8 | -55 01 46 | 4.57 | K3II | VAR:6.37 - 6.44P, 0.21R. | |||||||
HR 4066 | CD-47 5790 | 89736 | 221970 | 2831 | 10 20 16.7 | -47 41 57 | 5.65 | K5-M0III | |||||||||
HR 4074 | CP-55 3286 | 89890 | 237959 | W | A | 10 20 54.8 | -56 02 35 | 4.50 | B3IIIe v | 3.7 | 7.1 | D:AB binary?,VAR:Spectrum and H alpha vary. | |||||
HR 4080 | CD-41 5809 | 89998 | 221998 | 1268 | 4837 | 10 22 19.6 | -41 39 00 | 4.83 | K1III | ||||||||
HR 4087 | CD-41 5833 | 90170 | 222016 | 10 23 40.4 | -41 57 12 | 6.27 | G8IV | G:Epsilon Ind group. | |||||||||
HR 4093 | CD-41 5850 | 90393 | 222041 | 10 25 17.2 | -42 28 05 | 6.18 | G8III | ||||||||||
HR 4099 | CD-42 6222 | 90518 | 222047 | 10 26 09.5 | -42 44 20 | 6.13 | K1III | ||||||||||
HR 4107 | CP-54 3651 | 90677 | 238067 | 10 26 49.0 | -54 52 39 | 5.58 | K3II-III | ||||||||||
HR 4111 | CD-48 5655 | 90798 | 222081 | 4868 | 10 28 01.9 | -49 24 20 | 6.10 | K4III | VAR:Amp. (U-B), 0.13. | ||||||||
HR 4134 | CP-53 3909 | 91324 | 238146 | W | 10 31 21.8 | -53 42 56 | 4.89 | F6V | 3.5 | 46.4 | D:Companion K5, optical.,N:Called Y Argus in Velis by Lacaille 1763. Not the var. Y Vel. | ||||||
HR 4135 | CD-44 6583 | 91355 | 222126 | W | A | 10 31 57.5 | -45 04 00 | 5.74 | B6II | 0.4 | 13.7 | D:Fixed with HR 4136. Mag. and color for combined light, 5.16V, -0.15(B-V), -0.62(U-B). | |||||
HR 4136 | CD-44 6582 | 91356 | 222125 | W | B | 10 31 56.6 | -45 04 10 | 6.09 | B8II | 0.4 | 13.7 | D:See HR 4135. | |||||
HR 4139 | CD-43 6347 | 91437 | 222129 | 10 32 33.6 | -44 37 08 | 5.91 | G6-8III | ||||||||||
HR 4143 | CD-46 6205 | 91504 | 222136 | 1273 | W | 10 32 56.9 | -47 00 12 | 5.02 | K4III | 4.0 | 40.2 | D:CPM? Companion spectral class A. | |||||
HR 4154 | CD-43 6395 | 91805 | 222170 | W | 10 35 10.5 | -43 39 53 | 6.08 | G8II-IIICNVp | 8.4 | 14.7 | S:Weak G-band. | ||||||
HR 4167 | CD-47 6042 | 92139 | 222199 | I | W | 10 37 18.1 | -48 13 33 | 3.84 | F4IV+F3 | 0.9 | 0.3 | D:4.2 F3IV+F0V, 5.1 A6V, 16.30y, a = 0.340".,DYN:0.022".,S:Also classified A3m F0-F2.,SB:Primary of visual double, 10.2104d, K 42.3k/s, V0 +21.2k/s, msin3i 0.333, asini 5.11. | |||||
HR 4175 | CD-42 6390 | 92328 | 222222 | 2853 | W | 10 38 50.3 | -42 45 13 | 6.11 | Am+Am: | 0.1 | 0.2 | ||||||
HR 4180 | CP-54 3915 | 92449 | 238309 | 402 | W | 10 39 18.4 | -55 36 12 | 4.28 | G2-3Ib | 2.2 | 51.8 | D:Probably CPM. B is B8. C, 11.2v at 20" from B.,G:Red star Pleiades group. | |||||
HR 4216 | μ | CD-48 5913 | 93497 | 222321 | I | W | 10 46 46.2 | -49 25 12 | 2.69 | G5III+G2V | 3.7 | 1.7 | D:2.7 G5III, 6.4 G2V, 116.24y, a = 1.437". Secondary also classified F8:V:.,G:Sirius group? | ||||
HR 4221 | CP-56 3800 | 93563 | 238468 | Var? | 10 46 57.5 | -56 45 26 | 5.23 | B8-9IIIe v | M:Old disk population runaway star.,S:Variable H alpha.,VAR:Suspected amp. 0.08V on time scale of 2 hrs. | ||||||||
HR 4263 | CD-41 6220 | 94660 | 222422 | KQ Vel | 10 55 01.0 | -42 15 04 | 6.11 | A0pSiCr | S:Magnetic field.,VAR:Appears to be variable over long time scale, especially toward uv (may be constant in V). | ||||||||
HR 4274 | CD-50 5534 | 94985 | 238622 | 2874 | IW Vel | 10 57 07.9 | -50 45 54 | 5.91 | A4V | VAR:Amp. 0.02B, 0.150d. | |||||||
HR 4292 | CD-43 6692 | 95347 | 222485 | 10 59 59.4 | -43 48 26 | 5.81 | B8-9V | ||||||||||
HR 4293 | CD-41 6276 | 95370 | 222487 | 415 | 11 00 09.3 | -42 13 33 | 4.39 | A3IV | |||||||||
HR 4296 | CD-51 5220 | 95429 | 238674 | W | 11 00 08.6 | -51 49 04 | 6.15 | A3III-IV | 7.1 | 10.3 | |||||||
HR 4311 | CD-47 6466 | 96113 | 222538 | 2884 | 11 04 31.2 | -47 40 45 | 5.67 | A8III-IV | |||||||||
HR 4316 | CD-48 6157 | 96224 | 222548 | 11 05 04.2 | -49 23 33 | 6.13 | B9.5V |
Planetarische Nebel | ||||||||
---|---|---|---|---|---|---|---|---|
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 2792 | 09 12 26.5 | -42 25 39 | PN | 13.5 | 11.6 | 0.35 | ! planetary, pB = * 9, vS, R, am st | PK 265+4.1, ESO 314-PN6, AM 0910-421, CS=13.8 |
NGC 2899 | 09 27 03.0 | -56 06 20 | PN | 12.2 | 11.8 | 1.95 × 1 | F, pL, R, gmbM, am 80 st | PK 277-3.1, ESO 166-PN13 |
NGC 3132 | 10 07 01.8 | -40 26 10 | PN | 8.2 | 9.2 | 1.47 | !! planetary, vB, vL, lE * 9 m, 4s d | PK 272+12.1, ESO 316-PN27, AM 1004-401, CS=10.1, Eight-burst planetary |
Galaktische Nebel | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 2626 | 08 35 31.0 | -40 40 20 | EN+RN | 5 × 5 | * 9 inv in pB, pL, R neb | ESO 313-N*4 | ||
NGC 2736 | 09 00 17.0 | -45 56 53 | SNR | 20 × 2 | ! eeF, vL, vvmE 19° | ESO 260-N14, Herschel's Ray, Pencil Nebula | ||
Offene Sternhaufen | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 2547 | 08 10 09.0 | -49 13 30 | II2p | 4.7 | 25 | Cl, B, L, lC, st 7…16 | OCL 753, ESO 209-SC18, AM 0808-490 | |
NGC 2645 | 08 39 03.1 | -46 13 38 | II2p | 7.0 | 3 | Cl, S, st L and S | OCL 754, ESO 259-SC14 | |
NGC 2659 | 08 42 36.0 | -45 00 00 | III3m | 8.6 | 15 | Cl, L, Ri, pmE, st 11…14 | OCL 752, ESO 260-SC3 | |
NGC 2660 | 08 42 38.0 | -47 12 02 | I3m | 8.8 | 3 | Cl, pS, mC, iR, gbM, st 13…15 | OCL 759, ESO 260-SC4 | |
NGC 2669 | 08 46 19.0 | -52 56 06 | II3p | 6.1 | 14 | Cl, L, P, lC, st 10…13 | OCL 768, ESO 165-SC5 | |
NGC 2670 | 08 45 30.0 | -48 47 30 | II2p | 7.8 | 7 | Cl, pL, P, lC, st 13… | OCL 764, ESO 210-SC5 | |
NGC 2671 | 08 46 12.0 | -41 52 38 | I3p | 11.6 | 5 | Cl, pRi, lCM, st 12…13 | OCL 745, ESO 313-SC14 | |
NGC 2849 | 09 19 22.8 | -40 31 13 | II2m | 12.5 | 3 | eF, cL, R, vglbM, rr | OCL 756, ESO 314-SC13 | |
NGC 2866 | 09 22 06.5 | -51 06 08 | II2p | 20 | Cl, lC | OCL 774, ESO 212-SC3 | ||
NGC 2910 | 09 30 29.0 | -52 54 50 | I2p | 7.2 | 6 | Cl, cL, pRi, pC, st 10…14 | OCL 781, ESO 166-SC17 | |
NGC 2925 | 09 33 10.9 | -53 23 45 | III1p | 8.3 | 15 | Cl, pRi, pC, D * taken | OCL 783, ESO 166-SC22 | |
NGC 2972 | 09 40 11.5 | -50 19 13 | I1p | 9.9 | 5 | Cl, S, lRi, pC, st 13 | NGC 2999, OCL 778, ESO 212-SC11 | |
NGC 2982 | 09 42 00.0 | -44 01 36 | III1p | 12 | Cl, P, E, st 10…11 | OCL 770, ESO 262-SC1 | ||
NGC 3033 | 09 48 40.0 | -56 24 42 | II3p | 8.8 | 12 | Cl, pL, pRi, iF, st 11…12 | OCL 796, ESO 167-SC6 | |
NGC 3105 | 10 00 39.5 | -54 47 15 | I3p | 9.7 | 2 | Cl, C, lE, st 13…16 | OCL 798, ESO 167-SC14, AM 0958-543 | |
NGC 3228 | 10 21 22.0 | -51 43 42 | I1p | 6.0 | 5 | Cl, 9 L and a few S st | OCL 800, ESO 214-SC1 | |
NGC 3330 | 10 38 46.0 | -54 06 54 | II2p | 7.4 | 6 | Cl, P, st 9… | OCL 806, ESO 168-SC11 | |
NGC 3446 | 10 52 12.0 | -45 09 36 | OCL | 6.5 | Cl, pL, P, lC, iF, st 9…13 | ESO 264-SC45 | ||
IC 2391 | 08 40 18.0 | -52 55 00 | II3p | 2.6 | 60 | Cl, co, incl. ο Velorum 3.7 mag | OCL 767, ESO 165-SC4, Omikron Vel cluster | |
IC 2395 | 08 42 30.0 | -48 06 30 | II3p | 4.6 | 13 | Cl, co | OCL 763, ESO 210-SC3, vdB-Hagen 47 | |
IC 2488 | 09 27 27.0 | -56 57 24 | II2m | 7.4 | 18 | Cl, co | OCL 789, ESO 166-SC14 | |
Kugelsternhaufen | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 3201 | 10 17 36.8 | -46 24 38 | X | 6.9 | 20 | globular, vL, iR, lCM, st 13…16 | GCL 15, ESO 263-SC26 | |
Galaxien | ||||||||
Name | RA | Dec | Typ | bMag | vMag | Dim | Dreyer Beschreibung | Identifikation, Anmerkungen |
NGC 2845 | 09 18 36.9 | -38 00 35 | S0-a | 12.9 | 11.7 | 2.3 × 1.2 | vF, S, R, * 12 att sf | ESO 314-10, MCG -6-21-2, IRAS 09166-3747 |
NGC 3250 B | 10 27 44.5 | -40 26 08 | SBa | 13.7 | 12.7 | 2.2 × 0.6 | pB, pL, R, vgpsbM, * 13, 45° | ESO 317-29, MCG -7-22-9, AM 1025-401, IRAS 10255-4010 |
NGC 3256 | 10 27 51.4 | -43 54 19 | Sb/P | 12.2 | 11.5 | 3.8 × 2.1 | cB, S, R, gmbM | ESO 263-38, MCG -7-22-10, VV 65, AM 1025-433, IRAS 10257-4338 |
NGC 3256 A | 10 25 51.1 | -43 44 51 | SBm | 15.0 | 14.4 | 1.3 × 0.6 | cB, S, R, gmbM | ESO 263-34, AM 1023-432 |
NGC 3256 B | 10 29 01.1 | -44 24 12 | SBbc | 13.8 | 13.0 | 1.9 × 0.5 | cB, S, R, gmbM | ESO 263-39, MCG -7-22-14, IRAS 10268-4408 |
NGC 3256 C | 10 29 05.8 | -43 51 01 | SBcd | 13.3 | 12.6 | 1.7 × 1.2 | cB, S, R, gmbM | ESO 263-41, MCG -7-22-16, FAIR 431, AM 1026-433, IRAS 10269-4335 |
NGC 3261 | 10 29 01.4 | -44 39 27 | SBbc | 12.0 | 11.2 | 3.5 × 2.8 | F, S, R, am st | ESO 263-40, MCG -7-22-15, AM 1026-442, IRAS 10268-4423 |
NGC 3262 | 10 29 06.1 | -44 09 36 | SB0 | 14.2 | 13.2 | 1.1 × 0.7 | eF, S, R | ESO 263-42, MCG -7-22-17 |
NGC 3263 | 10 29 13.3 | -44 07 22 | SBc | 12.5 | 11.9 | 5.1 × 1.4 | F, S, mE 280°, psbM | ESO 263-43, MCG -7-22-18, AM 1027-435, IRAS 10270-4351 |
NGC 3283 | 10 31 11.2 | -46 15 02 | S0 | 12.5 | 11.5 | 3.2 × 1.5 | pF, S, R, gbM | ESO 263-48, IRAS 10290-4559 |
NGC 3318 | 10 37 15.0 | -41 37 38 | SBbc | 12.2 | 11.6 | 2.3 × 1.2 | cF, pL, pmE, lbM | ESO 317-52, MCG -7-22-26, AM 1035-412, IRAS 10350-4122 |
NGC 3318 A | 10 35 31.2 | -41 44 25 | SBc | 15.8 | 15.1 | 1.3 × 0.4 | cF, pL, pmE, lbM | ESO 317-50 |
NGC 3318 B | 10 37 33.3 | -41 27 58 | SBc | 13.9 | 13.2 | 1.5 × 1.1 | cF, pL, pmE, lbM | ESO 317-53, MCG -7-22-27, AM 1035-411, IRAS 10353-4112 |
NGC 3366 | 10 35 08.1 | -43 41 37 | SBb | 12.0 | 11.3 | 1.8 × 0.8 | F, E, gbM, * 6·7 v nr | IC 2592, ESO 264-7, MCG -7-22-24, IRAS 10329-4325, SAO 222170 (6.2) 1.5' n |
NGC 3482 | 10 58 34.2 | -46 35 03 | SBa | 13.2 | 12.4 | 1.9 × 1.4 | eF, S, R, gbM | ESO 264-56 |
PNG | RA J2000.0 | Dec J2000.0 | Main ID | PK | IRAS | Discoverer | Identities | oDiam ["] | rDiam ["] | Dist [kpc] | Rvel [km/s] | ExpVel [km/s] | C* Name | C* Mag | C* SP Type |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
PN G257.5+00.6 | 08 30 58 | -38 19 52 | VBRC 1 | VAN DEN BERGH et al 1973 | ESO 313-01, RCW 21, Wray 19- 11 | 61. | |||||||||
PN G258.1-00.3 | 08 28 28 | -39 23 43 | He 2- 9 | 258-00.1 | 08266-3913 | HENIZE 1964 | AS 200, ESO 312-05, MHa 392- 16, Sa 2- 26, Wray 16- 21 | 4.4 | AG82 101 | B: 17.55, V: 16.25 | |||||
PN G259.1+00.9 | 08 37 08 | -39 26 25 | He 2- 11 | 259+00.1 | HENIZE 1964 | ESO 313-05, Wray 16- 23 | 65. | B: >19.2, V: 18.9 | |||||||
PN G260.7+00.9 | 08 42 16 | -40 44 07 | Vo 3 | 08355-4027 | VOLK 1988 | PM 1-41 | 36. | ||||||||
PN G261.6+03.0 | 08 53 31 | -40 03 34 | He 2- 15 | 261+02.1 | 08516-3952 | HENIZE 1964 | AS 204, ESO 313-17, MHa 392- 12, Sa 2- 32, Wray 16- 32 | 24. | B: >17.7, V: >17.8 | ||||||
PN G262.6-04.6 | 08 23 54 | -45 31 10 | Wray 17- 18 | WRAY 1966 | ESO 259-06, LoTr 2 | 20. | |||||||||
PN G263.0-05.5 | 08 20 40 | -46 20 13 | PB 2 | 263-05.1 | 08190-4613 | PEIMBERT et al 1960 | ESO 259-04, He 2- 8, Sa 2- 24, Wray 16- 18 | 3. | |||||||
PN G263.2+00.4 | 08 48 39 | -42 53 46 | K 2-15 | 08470-4243 | KOHOUTEK 1971 | ESO 260-08 | 170. | AG82 108 | V: 11.3 | O(H) | |||||
PN G264.1-08.1 | 08 11 32 | -48 43 14 | He 2- 7 | 264-08.1 | 08100-4834 | HENIZE 1964 | ESO 209-19, StWr 3- 3, Wray 16- 16 | 45. | +88.0 ± 4.0 | 15.3 (O-III), 18.5 (N-II) | B: 16.8, V: 16.9 | ||||
PN G264.4-03.6 | 08 34 29 | -46 25 39 | Wray 17- 20 | WRAY 1966 | 60. : | ||||||||||
PN G265.1-02.2 | 08 43 24 | -46 08 29 | Ve 26 | 265-02.1 | 08417-4555 | VELGHE 1957 | ESO 260-05, He 2- 13, Sa 2- 31, Wray 16- 27 | < 5. | |||||||
PN G265.1-04.2 | 08 34 07 | -47 16 38 | ESO 259-10 | HOLMBERG et al 1978 | LoTr 3 | 28. | +49.0 ± 3.0 | 12.0 (O-III) | |||||||
PN G265.7+04.1 | 09 12 27 | -42 25 31 | NGC 2792 | 265+04.1 | 09105-4213 | HERSCHEL 1835 | ARO 507, ESO 314-06, He 2- 20, Sa 2- 36, VV 50, VV' 86, Wray 16- 36 | 13. | 2.6 | +14.0 ± 3.0 | 19.5 (O-III) | AG82 112, CD -41 4893, GCRV 6026, HD 79384 | B: 17.22 | ||
PN G268.4+02.4 | 09 16 10 | -45 28 46 | PB 5 | 268+02.1 | 09143-4516 | PEIMBERT et al 1960 | ESO 261-04, He 2- 24, Sa 2- 40, Wray 16- 39 | < 5. | AG82 115 | B: >19.7, V: 18.7 | |||||
PN G269.7-03.6 | 08 54 18 | -50 32 19 | PB 3 | 269-03.1 | 08527-5020 | PEIMBERT et al 1960 | ESO 211-04, He 2- 16, Sa 2- 33, Wray 16- 33 | 7. | |||||||
PN G272.4-05.9 | 08 53 37 | -54 05 08 | MeWe 1- 1 | MELMER et al 1990 | 110. | B: 19.4 | |||||||||
PN G273.2-03.7 | 09 08 41 | -53 19 08 | He 2- 18 | 273-03.1 | 09071-5307 | HENIZE 1964 | ESO 166-02, Sa 2- 35, Wray 16- 35 | 11. | +40.0 ± 19.0 | 15.0 (O-III) | |||||
PN G273.6+06.1 | 09 52 45 | -46 17 09 | HBDS 1 | HEBER et al 1984 | 90. | LSS 1362 | U: 11.11, B: 12.26, V: 12.47 | O(H) | |||||||
PN G274.1+02.5 | 09 41 10 | -49 22 42 | He 2- 34 | 274+02.1 | 09394-4909 | HENIZE 1964 | ESO 212-13, Wray 16- 56 | 0. | B: 18.2, V: 16.5 | ||||||
PN G274.3+09.1 | 10 05 46 | -44 21 44 | Lo 4 | LONGMORE 1977 | ESO 263-02 | 48. | +33.0 ± 20.0 | AG82 123 | B: 22.0, V: 20.5 | O(C) | |||||
PN G274.6+02.1 | 09 41 36 | -49 57 45 | He 2- 35 | 274+02.2 | 09398-4944 | HENIZE 1964 | ESO 212-14, Sa 2- 48, Wray 16- 57 | 5. | B: 16.4, V: 16.2 | WC ? | |||||
PN G274.6+03.5 | 09 47 24 | -48 58 19 | He 2- 37 | 274+03.1 | 09455-4844 | HENIZE 1964 | ESO 213-01, Sa 2- 50, Wray 16- 59 | 23. | +12.0 ± 5.0 | 30.7 (O-III) | |||||
PN G275.0-04.1 | 09 15 08 | -54 52 39 | PB 4 | 275-04.1 | 09136-5440 | PEIMBERT et al 1960 | ESO 166-06, He 2- 22, Sa 2- 38, Wray 16- 37 | 10.2 | AG82 114 | B: 15.97, V: 16.12 | |||||
PN G275.2-02.9 | 09 22 06 | -54 09 46 | He 2- 28 | 275-02.1 | 09205-5356 | HENIZE 1964 | ESO 166-09, Sa 2- 43, Wray 16- 44 | 10. | B: 17.6, V: 17.0 | ||||||
PN G275.2-03.7 | 09 18 01 | -54 39 29 | He 2- 25 | 275-03.1 | 09164-5426 | HENIZE 1964 | ESO 166-07, SaSt 1-2, Wray 16- 40 | 5. | AG82 116 | B: 17.08, V: 16.96 | |||||
PN G275.3-04.7 | 09 13 52 | -55 28 21 | He 2- 21 | 275-04.2 | HENIZE 1964 | ESO 166-05, Sa 2- 37, Wray 15- 344 | 2.4 | ||||||||
PN G275.5-01.3 | 09 30 49 | -53 09 57 | Pe 2- 4 | 275-01.1 | 09291-5256 | PEREK 1960 | ESO 166-18, He 2- 31, Sa 2- 46, VV' 90, Wray 16- 48 | 7. | |||||||
PN G275.8-02.9 | 09 24 45 | -54 36 20 | He 2- 29 | 275-02.2 | 09231-5423 | HENIZE 1964 | ESO 166-10, Sa 2- 44, Wray 16- 46 | 14. | +25.0 ± 6.0 | 23.6 (O-III) | |||||
PN G277.1-03.8 | 09 27 03 | -56 06 18 | NGC 2899 | 277-03.1 | 09255-5553 | HENIZE 1964 | ESO 166-13, Gum 27, He 2- 30, My 48, RCW 43, Sa 2- 45, Wray 16- 47 | 90. | +3.0 ± 4.0 | 23.5 (O-III), 25. (N-II) | B: >16.4, V: >15.9 | ||||
PN G277.7-03.5 | 09 31 27 | -56 17 41 | Wray 17- 31 | WRAY 1966 | ESO 166-21, RCW 44, Sa 3- 10, VBRC 2 | 110. | 28.0 (N-II) | ||||||||
PN G278.8+04.9 | 10 13 16 | -50 20 01 | PB 6 | 278+05.1 | 10113-5005 | PEIMBERT et al 1960 | ESO 213-07, He 2- 43, Sa 2- 58, Wray 16- 68 | 11. | B: 17.4, V: 17.6 | O VI,IUE spect, WC 3 | |||||
PN G279.6-03.1 | 09 43 26 | -57 17 00 | He 2- 36 | 279-03.1 | 09418-5703 | HENIZE 1964 | ESO 167-03, Sa 2-49, Wray 15- 428 | 22. | -7.1 ± 2.0 | AG82 120, CD -56 2932, CPD -56 2466, LS 1340 | B: 11.88, V: 11.30 | sdO + A2 III | |||
PN G280.0+02.9 | 10 11 58 | -52 38 15 | Ste 2-1 | 10100-5223 | STENHOLM 1975 | Sa 2- 56 | 20. : | ||||||||
PN G282.9+03.8 | 10 31 32 | -53 33 27 | He 2- 48 | 282+03.1 | HENIZE 1964 | ESO 168-05, Sa 2- 60, Wray 17- 45 | 14. | ||||||||
PN G283.3+03.9 | 10 34 18 | -53 40 58 | He 2- 50 | 283+03.1 | 10323-5325 | HENIZE 1964 | ESO 168-08, Sa 2- 62, Wray 16- 72 | 11.8 | +79.0 ± 19.0 | ||||||
PN G283.8+02.2 | 10 31 33 | -55 20 54 | My 60 | 283+02.1 | 10296-5505 | MAYALL 1951 | ESO 168-06, He 2- 49, PB 7, Sa 2- 61, Wray 16- 71 | 7.6 | AG82 128 | B: 17.6, V: 17.2 | |||||
PN G283.9+09.7 | 10 54 42 | -48 47 00 | ESO 215-04 | HOLMBERG et al 1978 | DS 1 | 300. | AG82 131bis, CD -48 6027, CPD -48 3606, KU Vel, LSS 2018 | U: 10.93, B: 12.09, V: 12.26 | sdO + MV, O(H) | ||||||
PN G285.4+01.5 | 10 38 32 | -56 46 33 | Pe 1- 1 | 285+01.1 | 10364-5631 | PEREK 1960 | ESO 168-10, He 2- 52, Sa 2- 64, VV'101, Wray 16- 75 | 3. | AG82 130 | WC 4-6 | |||||
PN G285.4+02.2 | 10 41 20 | -56 09 18 | Pe 2- 7 | 285+02.1 | 10393-5553 | PEREK 1960 | ESO 168-13, Sa 2- 66, VV' 103, Wray 16- 77 | 0. | |||||||
PN G285.7+01.2 | 10 39 32 | -57 06 10 | Pe 1- 2 | 285+01.2 | 10375-5650 | HENIZE 1964 | ESO 168-12, HFE 15, (He 2- 53), Sa 2- 65, VV' 102, , Wray 16- 76 | 5. | |||||||
PN G286.3+02.8 | 10 48 43 | -56 03 23 | He 2- 55 | 286+02.1 | 10466-5547 | HENIZE 1964 | ESO 169-03, Sa 2- 68, Wray 16- 79 | 18. | B: 17.6, V: 17.4 | WC 3 |