Sternbild Carina (Kiel des Schiffes)

Carina
Carina: IAU Sternbildkarte [150]

Eigenschaften

Das Band der Milchstraße verläuft durch den östlichen Teil von Carina und so findet man mit einem Fernglas viele Sternwolken und -haufen. Die Sterne iota und epsilon Carinae bilden zusammen mit kappa und delta Velorum das Falsche Kreuz, das oft für das Kreuz des Südens weiter östlich gehalten wird. Im Gegensatz zum echten zeigt das Falsche Kreuz nicht in Richtung südlichen Himmelspol. Carina schließt am Himmel eine Fläche von 494 Quadratgrad ein. Das Zentrum kulminiert jeweils etwa am 30. Januar um Mitternacht. [9, 15]

Sterne mit Eigennamen:

  • α Car: Canopus, Suhel, Suhail
  • β Car: Miaplacidus
  • ε Car: Avior
  • ι Car: Turais, Tureis, Scutulum, Aspidiske
Daten für das Sternbild Carina [150]
IAU NameCarina
IAU GenitivCarinae
IAU KürzelCar
Deutscher NameKiel des Schiffes
Saison (47° N)Nicht sichtbar
Rektaszension06h 02m 46s … 11h 20m 37s
Deklination-75° 41' 02" … -50° 45' 16"
Fläche494 deg2
Nachbarn (N↻)Vel, Pup, Pic, Vol, Cha, Mus, Cen
Sternbild Argo Navis
Sternbild Argo Navis: Illustration aus «Uranometria» von Johann Bayer, Kupferstich von Alexander Mair, 1603 [28]

Mythologie und Geschichte

Carina, der Schiffskiel, ist der südlichste Teil dessen, was früher einmal das prächtige, ausgedehnte Sternbild Argo Navis war, dem legendären Schiff von Jason und seinen Argonauten, die auszogen, das Goldene Vlies des Widders zu suchen. Mitte des 17. Jahrhundert wurde es aber vom französischen Astronomen Nicolas Louis de Lacaille in vier Teile auseinandergerissen - Carina, Puppis (Achterdeck), Pyxis (Schiffskompass) und Vela (Schiffssegel). Die hellsten Sterne der vier Teil-Sternbilder des Argo Navis besitzen immer noch eine durchgehende Bezeichnung mit griechischen Buchstaben, da Johann Bayer das Sternbild schon früher in seine Uranometria aufgenommen hatte. [7]

Ein interessantes Beispiel wo Sprache, Mythos und moderne Wissenschaft sich überschneiden: Himmelsnavigatoren der neusten Zeit verwenden Carinas hellsten Stern, Canopus, um ihre Raumsonden auf einem stabilen Kurs durch das Sonnensystem zu halten. Canopus eignet sich nicht nur wegen seiner Helligkeit (der zweithellste Fixstern) für diese Aufgabe, sondern er liegt auch nahezu auf der Normalen zur Ebene des Sonnensystems, d.h. nahe am südlichen Ekliptikpol. [87]

Kataloge

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 2278CP-52 90244267234430 06 17 51.7-52 43 596.41 K2-3III
HR 2322CP-52 91345291234475 06 23 37.7-52 10 525.98 G8III
HR 2326αCP-52 91445348234480245I 06 23 57.1-52 41 45-0.72 F0II G:Red star Pleiades group.,N:CANOPUS; Suhel; Suhail.,R:Diam. = 0.0061 - 0.0066".,S:Probable magnetic star.
HR 2341CP-52 91945509234488 06 24 48.2-52 48 236.51 K5-M0III
HR 2400CD-51 194646569234551 06 31 18.3-51 49 345.60 F8V
HR 2416CP-52 94747001234574 06 33 26.1-52 19 446.19 G8III
HR 2435CP-52 953473062345892508 06 34 58.6-52 58 324.39 A0II
HR 2513CP-52 99649396234693 06 45 26.1-52 12 046.57 G6Iab
HR 2515CP-52 99849517234699 06 45 53.7-52 24 365.80 K3III
HR 2523CD-51 207849689234705 06 46 52.8-51 15 575.40 K1II-III+G:p
HR 2524CP-54 111549705234704W 06 46 41.5-54 41 416.46 G6III 3.41.8
HR 2526CP-55 1063498772347102524 3220 06 47 18.7-55 32 245.61 K5III VAR:7.1 - 7.28B.
HR 2554CP-53 116850337234737 V415 Car06 49 51.3-53 37 204.40 G6II S:Secondary A0V and about 3 mag. fainter than primary.,SB:195.26d, K 24.9k/s, V0 +25.5k/s, asini 66.9.,VAR:From orbit based on IUE data, the star should be eclipsing with period 195.24d.
HR 2587CP-53 117751043234762 06 52 46.9-54 05 246.57 G5Ib-II
HR 2592CP-59 71651210234764 06 52 45.4-59 20 286.41 A3m SB:Small RV amp., nearly equal components.
HR 2634CP-55 111652603234826 06 58 39.6-55 43 466.27 K2III
HR 2638CP-56 121152622234825 06 58 36.2-56 23 416.45 F2II
HR 2652CD-51 2224530472348542544 Var?07 00 51.5-51 24 095.14 M1III VAR:Amp. 0.08V.
HR 2661CP-58 820533492348632546 3349 07 01 05.1-58 56 246.02 A8III VAR:Amp. 0.53:V.
HR 2674CP-58 82653921234890W 07 03 15.6-59 10 415.50 B9IV 0.81.6
HR 2683CP-56 123254118234902272 V386 Car07 04 18.3-56 44 595.17 A0pSi S:Magnetic field.,VAR:Amp. 0.026y, 3.275d.
HR 2698CD-51 230654732234940 07 07 13.3-51 58 045.96 K0III
HR 2754CP-62 78956239249774W 07 12 02.0-63 11 246.02 A0IV-V 0.40.4
HR 2767CP-52 112356705235040 07 15 21.0-52 29 595.97 K1III
HR 2813CP-52 115357852235110W A07 20 21.4-52 18 426.05 F0-2IV-V 0.69.3D:Binary with HR 2814.,DYN:0.027".
HR 2814CP-52 115357853235111W B07 20 21.7-52 18 356.60 G0V:e 0.69.3D:Binary with HR 2813.,DYN:0.027".,S:Sharp central CaII H and K emission.
HR 2815CD-51 244557917235116 07 20 38.7-52 05 105.39 B9II-III
HR 2862CD-50 2761592192351922575 07 26 21.9-51 01 065.10 K0III
HR 2884CP-52 119860060235239 07 29 59.6-52 39 045.87 K0III
HR 2892CP-54 1294602282352522586 07 30 30.9-54 23 585.96 M1III
HR 2925CD-51 257161031235310 07 34 39.5-51 28 296.28 A1III-IV
HR 2934CP-52 1231612482353361198 3661 07 35 39.7-52 32 024.94 K3III VAR:Amp. 0.02V.
HR 2941CP-55 128261394235343 07 36 01.7-55 53 156.39 K1-2IIICNII
HR 2971CP-52 124261966235391W V390 Car07 39 00.4-53 16 246.06 B9IV-Vp:Si: 7.815. VAR:Amp. >0.004y, 0.030u, 1.040d.
HR 3006CP-58 967627582354302600 07 42 10.2-58 37 516.43 B2.5V
HR 3012CP-57 130562897235440 07 42 53.3-58 13 486.21 K0III
HR 3031CP-56 142063382235490W 07 45 35.6-56 43 216.12 F0II 5.036.2
HR 3056CP-56 143763926235532W 07 48 19.2-56 28 166.33 K0III+A1V 2.21.1
HR 3062CP-56 144264067235539W 07 49 06.7-56 24 385.59 G5II 8.06.9
HR 3070CP-59 908641852499751206W 07 49 12.9-60 17 015.78 F1V 6.923.3D:Optical.
HR 3076CP-59 91064320235553 07 49 54.8-60 03 046.72 K0II
HR 3088CP-54 142064722235579 V372 Car07 52 29.7-54 22 025.70 B1.5IV VAR:Beta C Amp. 0.027V, primary period 0.1160d with secondary either 0.1168 or 0.1323d.
HR 3100CP-52 133365189235612 07 55 00.5-52 34 596.38 B8III
HR 3105CP-56 146865273235615 07 54 53.2-57 18 115.63 K3-4III G:Hyades group.
HR 3117χCP-52 134365575235635303 Chi Car07 56 46.7-52 58 563.47 B3IVp G:Sco-Cen assoc.,M:Soft X-ray source.,S:SiII strong for the spectral type.,VAR:Beta C, amp. 0.015V, 0.101d.
HR 3120CP-60 93565662250019 07 56 18.6-60 31 355.74 K3III G:NGC 2516 #119; Pleiades group.
HR 3126CP-58 102865750235638 V341 Car07 56 50.7-59 07 356.25 M0III eC:Strong IR excess probably due to carbon-rich material.,G:In reflection neb. IC 2220; in region of open cluster NGC 2516.,S:Emission feature at 10 and 20 micrometers attributed to silicate grains in circumstellar shell.,VAR:L 6.2 - 7.10V. IR observations of red giant in reflection nebula suggest star is losing mass and becoming a planetary,VAR:nebula. Circumstellar reflection nebula probably related to a hotter companion.
HR 3133CD-51 278465867235646 3841 07 58 21.4-51 26 556.44 A8-9IV S:Also classified F + K.,VAR:E?, 5.2 - 7.2p.
HR 3138CP-59 94465907250035IW 07 57 46.9-60 18 125.60 G0V 4.360. G:NGC 2516 #124.
HR 3139CP-62 92565908250030 07 57 12.5-63 17 496.14 B8V S:SrCr star.
HR 3147CP-60 100666194250055 V374 Car07 58 50.5-60 49 285.81 B2IVpne vG:In cluster NGC 2516 #134.,VAR:Gamma Cas 5.72 - 5.84V, period a few days. H alpha variable.
HR 3152CP-59 95466341250064 07 59 40.2-60 12 276.33 B5III G:NGC 2516 #136.
HR 3153CP-60 101866342250063 07 59 37.6-60 35 135.17 M1.5IIa G:NGC 2516 #110; Pleiades group.
HR 3156CP-53 1505664412356802622 08 00 49.9-54 09 055.87 B5Vn
HR 3157CP-54 147066546235686W 3871 08 01 22.9-54 30 546.10 B2IV-V 2.040.2D:Companion B9IIIp.,SB:Comp. A of visual double.,VAR:Amp. 0.15V.
HR 3159CP-63 866665912500692624 08 00 20.0-63 34 034.82 B3V G:Sco-Cen assoc.
HR 3161CP-55 141966607235690 08 01 31.5-55 27 186.28 B4V
HR 3180CP-52 137667364235735 08 05 04.0-53 06 295.53 K3-4III
HR 3186CP-62 95367536250101W V375 Car08 04 42.9-62 50 106.30 B2.5Vn e1.387.1D:Companion K0.,G:Sco-Cen assoc.,S:H alpha emission.,VAR:Beta C, amp. 0.04V, 0.264 or 0.359d?
HR 3217CP-63 89668423250127 08 08 24.5-63 48 046.28 B6Ve G:Sco-Cen assoc.
HR 3218CP-55 1467684342357842638 08 09 33.6-56 05 085.66 A3m
HR 3220CP-60 1074684562501312636 08 09 00.7-61 18 094.76 F5V
HR 3260CP-62 98569863250164W 08 15 15.9-62 54 575.16 A2V 2.63.9D:CPM, A2IV, F2V.,DYN:0.004".
HR 3274CP-58 109570267235872W 08 17 55.8-59 10 016.42 F5V 3.343.8
HR 3293CP-57 149070839235917 Var?08 21 12.0-57 58 235.97 B1.5III G:Sco-Cen assoc.; doubtful member of Sco-Cen cluster.
HR 3298CP-63 94070982250202 08 21 07.7-64 06 226.12 G6-8III
HR 3307εCP-59 103271129235932315 4058 08 22 30.8-59 30 351.86 K3III+B2:V N:Avior.,S:Also classified K0II + B2.,VAR:E? 1.82 - 1.94V, 3.57 - 3.83p, 785:d.
HR 3349CP-54 164771919236001W 08 27 27.4-55 00 426.53 A0V 0.00.2
HR 3368CP-54 166772322236032W 08 29 36.3-55 11 286.36 G0V 5.92.4
HR 3414CP-57 159173389236106 08 35 19.6-58 00 334.86 K0III
HR 3415CP-57 159073390236105 08 35 15.4-58 13 305.26 B3V+B3Vn G:Sco-Cen assoc.
HR 3432CP-62 1058738872502882679W 08 37 18.8-62 51 135.47 K0III 5.67.6
HR 3443CP-59 107574148250291W 08 39 13.2-60 19 026.36 A0V 0.61.2
HR 3455CP-57 164474341236179W 08 40 43.6-57 32 436.34 A3V 1.93.8
HR 3457CP-59 1080743752361812685W V343 Car08 40 37.0-59 45 404.33 B1.5III 8.915.7SB:133.92d.,VAR:Beta C 4.3 - 4.33V, amp. 0.04B.
HR 3471CP-55 168874622236206 08 42 20.9-55 46 276.29 K2III
HR 3489CP-58 120275086236241W A08 45 05.3-58 43 306.21 B7III 0.14.1D:Components B8III and B7IV. Component B, RV +24k/s.
HR 3498CP-56 1865753112362682695 V344 Car08 46 42.5-56 46 114.49 B3Vne vG:Sco-Cen assoc.,VAR:Gamma Cas 4.4 - 4.50V. Variable H alpha.
HR 3536CP-57 175976113236339 08 51 36.6-57 38 015.59 B8III
HR 3549CP-56 191876346236368 08 53 03.8-56 38 586.03 A0V
HR 3560CP-59 117476538250369 08 53 48.7-60 21 155.78 B5III
HR 3568CP-57 179076640236402 08 54 54.0-58 14 246.38 B5V
HR 3571CP-60 124376728250374336W 08 55 02.8-60 38 413.84 B8-9II 8.821.1G:Member of the local association (Pleiades group).
HR 3582CP-58 1301770022364361233W AV376 Car08 56 58.4-59 13 464.92 B2IV-V 1.940.2D:Fixed. B is B9.5V. vsini both components 0k/s.,G:Sco-Cen assoc.; member of Pleiades group.,VAR:Beta C 4.91 - 4.96V, amp. 0.015b, 0.0208d.
HR 3598CP-58 132777370236475W 08 59 24.1-59 05 015.16 F3V 6.826.2D:Optical.,G:Hyades group.
HR 3604CP-60 128377615250417 09 00 45.7-60 57 505.79 G8II
HR 3622CP-57 185978293236578W 09 04 48.0-57 51 096.44 A8III 3.63.3D:Binary.
HR 3632CP-63 109378632250441 09 06 07.6-64 29 596.37 K3III
HR 3642CP-70 86178764256583 V345 Car09 05 38.3-70 32 204.71 B2IVe S:Shell star.,VAR:Gamma Cas 4.67 - 4.78V.
HR 3643CP-72 779787912565822720 09 05 08.8-72 36 104.48 F9II
HR 3659CP-58 141979351236693 V357 Car09 10 58.0-58 58 013.44 B2IV-V eG:Sco-Cen cluster; member of Pleiades group.,N:a Car.,S:H alpha emission.,SB:6.7447d, K 21.5k/s, V0 +23.3k/s, asini 1.96. Equal components.,VAR:E 3.41 - 3.44V, 3.20 - 3.56p, 0.05R, 6.751154d.
HR 3663CP-61 120179447250471 09 11 16.6-62 19 023.97 B3III vG:Sco-Cen assoc.; probable member of Sco-Cen cluster. See HR 2702.,VAR:Helium var.?
HR 3673CP-58 143279698236723 09 12 55.6-59 24 525.54 G6II
HR 3685βCP-69 102380007250495348 09 13 12.0-69 43 021.68 A2IV vN:Miaplacidus.,R:Diam. = 0.00151 - 0.00159".,VAR:Balmer lines show quasi periodic var. in cycles of about 35 min.
HR 3691CP-57 194980094236772 Var?09 15 17.5-58 23 196.02 B7IV G:Sco-Cen assoc.,VAR:Amp. 0.04b.
HR 3693CP-57 195180126236777 09 15 35.0-57 34 416.32 G8II
HR 3696CP-57 196180230236787 4440 09 16 12.2-57 32 294.34 M1III
HR 3699ιCP-58 146580404236808351 4444 09 17 05.4-59 16 312.25 A8Ib N:Turais; Tureis; Scutulum; Aspidiske.,VAR:2.2 - 2.5:v.
HR 3712CP-68 91880671250526W 09 17 17.2-68 41 225.39 F4V 0.00.1D:AB 6.1 F4V, 6.1, 3.2y, a = 0.124".
HR 3713CP-66 100280710250529 09 17 51.7-67 03 036.11 K2III
HR 3720CP-74 57980951256599W 09 17 25.4-74 53 405.29 A1V 0.50.2D:AB binary. C, 10.0v at 7", CPM?
HR 3721CP-74 58080950256600 09 17 27.4-74 44 055.86 A0V
HR 3728CP-61 1242811012505442745 09 20 56.8-62 24 174.81 G6III
HR 3740CP-59 137481502250561 09 23 27.4-60 18 096.30 K1-2II-III
HR 3742CP-61 126581613250563 09 24 05.7-61 38 565.99 K0III
HR 3752CP-61 127181830250575W 09 25 27.1-61 57 015.77 A4V 4.58.7D:CPM.,G:Hyades group.
HR 3761CP-64 103782068250583 09 26 44.2-64 55 476.05 A3Vn
HR 3776CP-61 127782347250590 09 28 47.0-62 16 235.92 K1III
HR 3777CP-71 83382350256623 09 27 06.4-71 36 085.47 K2III G:Hyades group.
HR 3783CP-66 1018824062505912754 09 28 30.6-66 42 075.91 A0V
HR 3793CP-57 209082536237056W 4516 09 30 23.4-58 21 425.88 M2III 7.72.3C:V magnitudes scatter from 5.70 to 5.94.
HR 3813CP-66 102582858250611 09 31 32.9-66 43 106.27 K1III
HR 3816CP-62 125382901250614IW R Car09 32 14.6-62 47 206.10 M6-7IIIep v7.32.1S:Also classified M4e-M8e.,VAR:Component A of visual double. M 3.9 - 10.1v, 308.71d.
HR 3821CP-72 83583095256634362 09 31 36.3-73 04 515.47 K4III
HR 3825CP-58 157683183237117 09 34 26.7-59 13 464.08 B5II G:Member of Pleiades group.
HR 3841CP-64 104983523250636 09 36 05.1-64 57 026.56 A2V
HR 3856CP-60 147783944250653 4577 09 39 21.0-61 19 414.52 B9IV-V G:Pleiades group; Sco-Cen assoc.,VAR:4.4 - 4.44B.
HR 3863CP-57 222884121237221W 09 40 42.5-57 59 015.32 A3IV 0.20.2D:6.0 A2, 6.1, 10.72y, a = 0.142". Combined mag., colors.,DYN:0.019".,SB:Primary of visual double.
HR 3864CP-56 243584152237224 09 41 02.2-57 15 355.80 K0-1III
HR 3883CP-56 249984809237314 4623 09 45 40.5-57 11 086.46 B8III-IV VAR:6.5 - 6.59V.
HR 3884CP-61 1333848102506831254 l Car09 45 14.8-62 30 283.69 G5Iab-Ib vRV:35.5374d.,S:Possible circumstellar shell. Also classified F6Ib-K0Ib.,VAR:CDelta 3.28 - 4.18V, 35.53584d. Period varies.
HR 3887CP-58 164084850237321 09 45 55.4-58 47 396.22 F5IV
HR 3890υCP-64 108485123250695W A09 47 06.1-65 04 193.01 A6Ib 3.05.0D:CPM with HR 3891. Mag. and colors for combined light, 2.96V, +0.27(B-V), +0.12(U-B), +0.29(R-I).,RV:Probably blended with HR 3891.
HR 3891υCP-64 108485124250696W B09 47 06.7-65 04 216.26 B7III 3.05.0D:See HR 3890.,DYN:0.003".,RV:Probably blended with HR 3890.
HR 3913CP-58 1673856552374182789 09 51 12.1-59 25 335.79 K2IVCNIV-Vp
HR 3914CP-62 133585656250721 09 50 55.7-62 44 435.57 K1IIICNII
HR 3944CP-70 953866062566722799 09 56 09.7-71 23 226.35 B9Ib
HR 3948CP-63 1233866342507602801 09 57 15.2-64 29 226.58 K0-1III
HR 3949CP-68 101186659250761 09 56 59.7-69 06 076.20 B3V G:Sco-Cen assoc.? Probable member of Sco-Cen cluster.
HR 3957CP-56 277087238237621 10 01 58.0-57 20 596.20 K1II
HR 3960CP-59 169587283250782 10 02 00.0-60 25 155.94 A9IV G:In cluster NGC 3114 #48.,S:Also classified F0II, F2II, F2III-IV.
HR 3966CP-59 175287436237640 10 02 59.9-60 10 436.19 A6II-III G:NGC 3114 #125.
HR 3967CP-61 143187438250789 4720 10 02 49.4-62 09 236.42 K3Ib
HR 3971CP-61 144187543250795W 10 03 34.3-61 53 026.14 B7IVne 1.51.2RV:Probably corresponds to circumstellar shell.,S:Shell star.
HR 3995CP-65 124888323250836W 10 08 42.6-65 48 555.28 K0III 4.263.3
HR 3999CP-60 170188366250840 S Car10 09 21.9-61 32 575.60 M2-3IIIe S:Also classified K5e-M6e.,VAR:M 4.5 - 9.9v, 149.49d.
HR 4002CP-68 103488473250844W 10 09 30.5-68 41 005.81 A0IV 0.10.8
HR 4007CP-58 197988647237773 V368 Car10 11 35.2-58 49 416.40 M3III VAR:Lb? 6.1 - 6.40v.
HR 4009CP-57 2781886612377762819 QY Car10 11 46.5-58 03 385.72 B2IVpne vM:Suspected hard X-ray source.,S:Strong variations in H alpha line widths.,VAR:Gamma Cas 5.63 - 5.83V.
HR 4018CP-59 197488825237799 10 13 01.3-59 55 056.10 B4Ve S:H beta weak emission.
HR 4022CP-61 1517889072508752822 10 13 21.2-61 39 326.41 B2V G:Sco-Cen assoc.; doubtful member of the Sco-Cen cluster. On the basis of RV and proper motion HR 4022 and several fainter,G:stars are possibly associated with l Car.
HR 4025CP-65 127388981250880 10 13 30.6-66 22 235.16 Am S:K/H/m indicate A5/A7/F0II-III, respectively.
HR 4037ωCP-69 117889080250885385 10 13 44.2-70 02 173.32 B8III tG:Sco-Cen assoc.,S:Shell star. Variable H alpha.
HR 4043CP-59 200889263237853W 10 16 03.1-59 54 126.22 A5V 0.10.4D:6.9 A5V, 7.0 A5V, 124.0y, a = 0.435". Combined mag., color.
HR 4050CP-60 1817893882509051264W V337 Car10 17 05.0-61 19 563.40 K3IIa 9.216.4VAR:Lc? 3.36 - 3.44V.
HR 4065CP-64 124889715250917W 10 19 04.8-64 40 355.67 A1V 0.12.4D:CPM? Combined mag., colors. Components A1V and A1Vn.,RV:Component B, +19k/s.
HR 4089CP-66 1243902642509402834 10 22 58.1-66 54 064.99 B8V vS:Helium-weak star.,SB:0.9445d, 1.0565d or 17.7d.,VAR:Possible He var.
HR 4091CP-57 312790289238021 4846 10 23 50.9-57 57 146.35 K4III
HR 4095CP-57 316490454238046 10 24 59.4-58 34 355.95 F2III
HR 4102CP-73 73390589256710391 4856 10 24 23.7-74 01 544.00 F2IV
HR 4105CP-73 73590630256711 10 24 44.3-73 58 186.19 A2-3V
HR 4110CP-57 325690772238077 V399 Car10 27 24.4-57 38 204.66 A9Ia G:Cluster IC 2581 #1; Car OB1.,S:Variously classified A5Ia through F0Ia and F7Ia-O.,VAR:Amp. 0.07B, 0.06(B-V), 0.14(U-V), 58.82d.
HR 4114CP-58 222790853238085393 4869 10 27 52.7-58 44 223.82 F2II VAR:3.79 - 3.83V.
HR 4115CP-65 135490874250966 10 27 25.3-65 42 176.01 A2V
HR 4120CP-63 144091056250979 10 28 52.6-64 10 205.29 M0III S:Also classified K3Ib.
HR 4128CP-60 194591270250992W 10 30 39.2-61 21 226.43 M2IIIe 1.282.6D:B = CPD-60d1944 = HD 91269, 7.54V, -0.08(B-V), -0.57(U-B), B5Vne, shell star.,N:In the HD the magnitudes for HD 91269, 91270 had been interchanged, leading to much subsequent confusion between the red,N:and blue components.
HR 4129CP-66 129191272250989 4881 10 30 08.7-66 59 066.19 B4IV
HR 4138CP-71 1034913752567222842 10 30 20.1-71 59 354.74 A1V S:Also classified Am, A2m, A2III.
HR 4140CP-61 170491465251006397 PP Car10 32 01.4-61 41 073.32 B4Vne vS:Shell star. Variable Balmer line profiles. Indications that stellar wind is stronger than in most early-type Be stars.,VAR:Gamma Cas 3.27 - 3.37V.
HR 4142CP-72 98191496256723W 4886 10 31 02.0-73 13 184.93 K4-5III 7.632.0S:Also classified K4Ib and M1III.
HR 4144CP-58 228591533238168 10 32 47.6-58 40 016.00 A2Iab G:Sco-Cen assoc.; in reflection nebula Car R1, probably connected with Carina nebula NGC 3372; Car OB1.
HR 4147CP-57 343191619238182 V369 Car10 33 25.3-58 11 256.14 B7Iae vG:Car OB1.,S:H alpha emission variable.,VAR:Alpha Cyg, amp. 0.1v, 0.05y, cycles 15 - 20d? Irregular var. in H alpha emission profiles indicating chromospheric,VAR:activity.
HR 4151CP-60 198391767251014 4898 10 34 12.9-60 59 166.23 K2-3III VAR:Amp. 0.08(B-V).
HR 4159CP-56 354491942238222 4904 10 35 35.3-57 33 284.45 K3-4II
HR 4164CP-58 237192063238242 4909 10 36 20.3-59 33 535.08 K1III
HR 4169CP-58 241192207238271 V370 Car10 37 26.8-58 44 005.45 A0Iae vG:Car OB1; member NGC 3324, a very young open cluster; Sco-Cen assoc.,M:Possible abs. mag. = -8.0V.,S:Shell star. H alpha emission.,VAR:Alpha Cyg 5.45 - 5.52V, amp. 0.035y.
HR 4173CP-56 358892287238278 10 38 02.5-57 15 235.91 B3IV G:Sco-Cen assoc.
HR 4177CP-58 246092397238295W 4922 10 38 45.1-59 10 594.66 K4-5III: 3.414.6D:Fixed. Combined mag., colors. Companion A5V.,S:Also classified K1II, K4Ib-II, K5Ib.
HR 4179CP-58 247492436238304W 10 38 59.4-58 49 015.92 M1III 2.723.5D:Optical.
HR 4185CP-64 140392664251059 V364 Car10 40 11.3-65 06 025.52 B9pSi D:Lambda 4200 star.,G:IC 2602 #27.,VAR:Alpha CV 5.48 - 5.52V, 1.6731d. Magnetic field varies with same period. Relative to HR 4205, delta u = 0.102,,VAR:delta y = 0.046.
HR 4186CP-73 75892682256742 10 39 16.6-74 29 376.07 K3II
HR 4188CP-59 245092740238353 4939 10 41 17.6-59 40 376.42 WN7-A G:HII region.,M:One of only four WR stars bright enough to have been observed spectroscopically in UV by COPERNICUS.,S:Here A means narrow lines, not an A-type spectrum.,SB:10.04d, K 140k/s, V0 +75k/s, asini 19.3 (period questioned). Alternate orbits 80.35d, K 77k/s, V0 -28k/s;,SB:80.35d, K 70k/s, V0 var.
HR 4196CP-63 158992938251078 10 42 14.0-64 27 594.82 B4V G:IC 2602 #33.
HR 4198CP-58 258192964238379 4948 10 42 40.6-59 12 575.38 B2.5Iae vG:Car OB1; in cluster CR 228; nebulosity.,S:H alpha varies.
HR 4199θCP-63 159993030251083406I 10 42 57.4-64 23 402.76 B0Vp vC:Color excess E(B-V) = +0.06.,G:In cluster IC 2602 #37.,S:Lyman beta observed from COPERNICUS. Nitrogen enhanced. Moderately He-rich.,VAR:Spectrum var., 1.7788d. Discussion of earlier suspected period of 0.7045d given by Walborn (1979, PASP, 91, 442).,VAR:vsini 202k/s. High speed mass ejection.
HR 4200CP-59 253293070251090 4951 10 43 32.1-60 34 004.57 K4III S:Also classified K3Ib.
HR 4204CP-63 161993163251095 Var?10 43 51.2-64 14 565.77 B2.5V G:IC 2602 #40, nonmember.,VAR:Amp. 0.028y, 0.038u, possibly eclipsing. Intervals between minima about 3d.
HR 4205CP-63 162393194251096 10 44 06.9-63 57 404.82 B5Vn G:IC 2602 #41; Sco-Cen assoc?,M:Old disk population runaway star.
HR 4210ηCP-59 262093308238429IW Eta Car10 45 03.6-59 41 036.21 pec 0.10.2C:Infrared color excess.,G:HII region R51; may be member of cluster TR 16.,VAR:Comp. A of double. SN? S Dor type, -0.8 - 7.9v. Abs. mag. -14 in 1843. Massive star surrounded by expanding gas and,VAR:dust shell; soft X-ray source.
HR 4211CP-70 118393344256750W A10 44 19.4-70 51 366.26 A5IV-V 0.263.0D:CPM with HR 4212.
HR 4212CP-70 118593359256751W B10 44 32.1-70 51 186.46 A6IV 0.263.0D:CPM with HR 4211.
HR 4213CP-71 111893372256752 10 44 26.5-72 26 386.27 F6V
HR 4217CP-59 267193502251113W 10 46 16.8-60 36 126.25 A0IV 7.84.2SB:Comp. A of visual double. Equal components.
HR 4219CP-63 164693540251115 10 46 16.5-64 30 545.34 B6V eG:IC 2602 #48.,S:Possible H alpha emission.
HR 4220CP-63 164993549251117W 10 46 29.7-64 15 485.23 B7IV 0.10.1G:IC 2602 #49.
HR 4222CP-63 165593607251120 10 46 51.2-64 23 004.85 B3IV G:IC 2602 #51; member of the local association (Pleiades group); Sco-Cen assoc.
HR 4226CP-56 382193662238480 4975 10 47 38.7-57 28 046.36 M1II VAR:Amp. 0.09 in (B-V).
HR 4228CP-59 2720937372384932862 10 48 05.4-59 55 096.00 A0Ia-Iab G:Car OB1.
HR 4239CP-58 275593943238514W 10 49 24.1-59 19 255.91 B9.5IV-V 1.21.1
HR 4250CP-56 3947943672385572868 10 52 30.9-57 14 265.25 B9Ia eS:H alpha emission.
HR 4257CP-58 283494510238574W 5011 10 53 29.6-58 51 123.78 K1III 2.7153.9VAR:3.76 - 3.80V.
HR 4262CP-70 124694650256770W 10 53 42.0-70 43 135.99 B6V e0.61.5S:H alpha emission.
HR 4266CP-61 196094683251173W 10 54 29.6-61 49 365.93 K4III 5.07.1
HR 4271CP-59 284094776251178 T Car10 55 17.2-60 31 015.92 K0III VAR:Cst? 7.00B.
HR 4276CP-59 288895109238635 U Car10 57 48.4-59 43 556.11 G3Ia VAR:CDelta 5.72 - 7.02V, 38.7681d since 1939. Period varies, earlier 38.753d.
HR 4279CP-74 755952082567752875 10 57 15.7-75 05 596.13 K1II
HR 4290CP-60 243395324251205W 10 59 14.0-61 19 136.16 B8IV 3.54.1
HR 4323CP-58 311296544238779W 5091 11 06 29.3-58 40 316.02 K2II-III 5.912. VAR:7.2 - 7.37B.
HR 4325CP-61 206796566251269 11 06 32.4-62 25 274.61 G8III
HR 4326CP-64 163096568251267 11 06 24.2-64 50 236.41 A3V
HR 4329CP-70 1305967062568001288W Var11 06 49.9-70 52 415.57 B2V 8.215. G:Sco-Cen assoc.,VAR:Amp. 0.02b.
HR 4337CP-58 3189969182388131289I V382 Car11 08 35.4-58 58 303.91 G40-Ia vG:Car OB2; NGC 3532.,S:Also classified F8Ia-G2Ia.,VAR:Delta Cep? 3.84 - 4.02V.
HR 4338CP-61 2075969192512862891 V371 Car11 08 34.0-61 56 505.13 B9Ia tS:H alpha emission variable.,VAR:Alpha Cyg 5.12 - 5.19V, amp. 0.055y, 15 - 20d cycles. Also var. H alpha profiles indicating chromospheric activity.
HR 4342CP-57 438797271238839 11 10 54.7-58 27 196.88 B7III
HR 4349CP-70 133697472256808 11 11 29.5-71 26 116.35 K2-3III
HR 4352CP-59 319097534251316W 5137 11 12 36.0-60 19 034.60 A6Iae 6.821.7D:Fixed sep.,G:Car OB2; probable member of NGC 3572a.,S:Also classified F0Ia.,VAR:Component A of double; Cep?, 4.58 - 4.62V.
HR 4355CP-63 1860975832513202893W 11 12 45.2-64 10 115.23 B8V 6.719.1D:Companion A0, optical.
HR 4361CP-58 331597670238877 Var11 13 30.8-59 37 105.74 B1.5V G:Member of the local association (Pleiades group).,VAR:Amp. 0.03b, 0.58:d.
HR 4379CP-67 1703982922513412903W 5163 11 17 19.0-67 49 256.06 M2III 7.534.7VAR:6.0 - 6.6V.
HR 4384CP-63 188198560251357 11 19 16.5-64 34 575.99 F6IV

Revised+Historic NGC/IC, Version 22/9, © Dr. Wolfgang Steinicke [277]
Planetarische Nebel
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 286709 21 25.4-58 18 40PN9.79.70.4!! planetary = * 8, vS, R, * 15, 59° 13"PK 278-5.1, ESO 126-PN8, CS=13.6
NGC 321110 17 50.4-62 40 12PN11.810.70.32planetary = * 10, R, am 150 stPK 286-4.1, ESO 127-PN15, AM 1016-622
IC 244809 07 06.5-69 56 29PN11.510.40.45Planetary, stellPK 285-14.1, ESO 61-PN1, AM 0906-694, CS=14.0
IC 250109 38 47.3-60 05 29PN11.310.40.03Planetary, stellPK 281-5.1, ESO 126-PN26, CS=14.0
IC 255310 09 20.9-62 36 47PN13.010.30.15Planetary, stellarPK 285-5.1, ESO 127-PN10, CS=12.9
IC 262111 00 20.2-65 14 56PN11.311.20.08Planetary, stell, 10.5 magPK 291-4.1, ESO 93-PN4, CS=13.6
Galaktische Nebel
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 319910 17 24.0-57 55 18EN20 × 15! vB, vL, falcate, D * invESO 127-EN14
NGC 332410 37 19.3-58 38 03EN16 × 14pB, vvL, iF, D * invESO 128-EN6
NGC 337210 45 06.0-59 52 00EN3.0120 × 120! Great neb, η ArgûsESO 128-EN13, Eta Car nebula
NGC 350311 01 17.2-59 50 50EN+OCL3 × 33 S st 10 m in vF nebOCL 833, ESO 128-EN28, AM 1059-593
NGC 357611 11 32.7-61 21 44EN3 × 3F, lE, 1st of 6ESO 129-EN5, with N 3579
NGC 357911 11 59.6-61 14 35EN20 × 15F, lE, sbM, 2nd of 6ESO 129-EN8, with N 3576
NGC 358111 12 01.9-61 18 06EN* 12 with fan-shaped neb att, 3rd of 6ESO 129-EN9, AM 1109-610
NGC 358211 12 11.9-61 16 24ENB, bM*, 4th of 6ESO 129-EN10
NGC 358411 12 19.8-61 13 42ENF, L, E 0°, bM, 5th of 6ESO 129-EN12
NGC 358611 12 29.9-61 21 08ENeF, S, E 160° ±, 6th of 6ESO 129-EN13
IC 222007 56 51.3-59 07 31EN+*5 × 5!! L, E, spiral, * inv.ESO 124-RN?3, AM 0755-585, Butterfly/Toby Jug nebula
IC 259910 37 27.0-58 44 00EN* 8.5 in neb, 3324 f 6s, 6' spart of NGC 3224
Offene Sternhaufen
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 251607 58 04.0-60 45 12I3r3.83.822Cl, vB, vL, pRi, st 7…13OCL 776, ESO 124-SC6
NGC 260908 29 30.0-61 06 36OCL6Cl, pS, lRi, lCESO 124-SC17
NGC 303609 49 15.9-62 40 32OCLCl, cL, lCESO 126-SC27
NGC 311410 02 36.0-60 06 00II3r4.235Cl, eL, lC, B, st 9…14OCL 802, ESO 127-SC2
NGC 324710 24 12.0-57 45 48II2p8.07.65st inv in nebOCL 809, ESO 127-SC19, Westerlund 2, in EN
NGC 325510 26 31.3-60 40 42I3m11.02Cl, pS, vC, st 15OCL 817, ESO 127-SC20
NGC 329310 35 51.0-58 13 48I3r4.75Cl, B, Ri, pLOCL 816, ESO 128-SC5, Gem cluster
NGC 349610 59 36.0-60 20 12III1m8.27Cl, pL, pRi, lC, st 13OCL 836, ESO 128-SC26
NGC 351911 04 02.7-61 22 05III2p7.78Cl, pRi, pCOCL 844, ESO 128-SC30
NGC 353211 05 40.0-58 44 00II1m3.23.050!!, Cl, eL, R, lC, st 8…12OCL 839, ESO 128-SC31
NGC 357211 10 26.6-60 14 38I2m6.67Cl, pRi, lCOCL 846, ESO 129-SC1
NGC 359011 12 58.9-60 47 20II1p8.22Cl, pRi, C, EOCL 852, ESO 129-SC14
NGC 360311 15 06.6-61 15 40I1pn9.14globular and neb, st 15…18OCL 854, ESO 129-SC16
IC 258110 27 26.1-57 37 32I3m4.35Cl, around * 5.4 magOCL 811, ESO 168-SC3
IC 260210 42 56.5-64 23 39II3m1.6100Cl, co, incl. θ CarinaeOCL 838, ESO 93-SC2, Southern Pleiades
IC 271411 17 22.0-62 43 18II3m8.215Cl, pCOCL 855, ESO 129-SC18
Kugelsternhaufen
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 280809 12 02.6-64 51 45I6.214! globular, vL, eRi, vgeCM 45s d, st 13…15GCL 13, ESO 91-SC1
Galaxien
NameRADecTypbMagvMagDimDreyer BeschreibungIdentifikation, Anmerkungen
NGC 219106 08 23.7-52 30 44SB012.311.41.7 × 0.9pB, vS, E, vsbM, * 9 p 5sESO 160-14
NGC 236907 16 37.7-62 20 38SBa13.212.33.5 × 1.1pB, pL, iE, glbMESO 122-18, AM 0716-621, IRAS 07160-6215
NGC 2369 A07 18 43.5-62 56 12SBbc13.712.91.8 × 1.2pB, pL, iE, glbMESO 88-8, AM 0718-625, IRAS 07182-6250
NGC 2369 B07 20 29.7-62 03 14SBbc14.013.21.5 × 1.4pB, pL, iE, glbMESO 123-5, IRAS 07199-6157
NGC 238107 19 57.4-63 04 01SBa13.612.81.4 × 1.4vF, vS, R, am stESO 88-10, FAIR 266, AM 0719-625, IRAS 07194-6258
NGC 241707 30 12.1-62 15 09Sbc12.812.02.8 × 1.9vF, L, R, gbM, RESO 123-15, AM 0729-620, IRAS 07295-6208
NGC 250207 55 51.5-52 18 25SB013.212.02.1 × 1.3pF, S, R, vgpmbMESO 209-8, AM 0754-521
NGC 264008 37 24.7-55 07 25E/SB012.111.12.2 × 1.9pB, S, R, 3 or 4 vS st p nrESO 165-2, IRAS 08360-5456
NGC 271408 53 29.8-59 13 03E013.912.91.1 × 1.1eF, S, R, pslbMESO 125-7
NGC 278809 09 03.3-67 55 57Sab13.112.31.8 × 0.4vF, vS, mE 105°ESO 61-2, AM 0908-674, IRAS 09083-6743
NGC 282209 13 49.8-69 38 39E311.910.93.3 × 2.2pF, vS, R, glbMESO 61-4, IRAS 09132-6926, Beta Car (1.7) 5' sp
NGC 283609 13 45.3-69 19 59Sbc12.611.82.7 × 2F, pS, R, glbMESO 61-3, IRAS 09131-6907
NGC 284209 15 36.4-63 04 10SB0-a13.412.51.6 × 1.3F, vS, bet 2 stESO 91-4, FAIR 282, IRAS 09144-6251
NGC 288709 23 24.3-63 48 44E-S012.811.72.1 × 1.6F, S, R, pmbM, B * nrESO 91-9, AM 0922-633
NGC 305909 50 08.0-73 55 17SBbc11.711.03.6 × 3.2F, L, iR, glbM, S * invESO 37-7, IRAS 09496-7341
NGC 313610 05 48.2-67 22 39E311.710.73.1 × 2.1pB, pS, R, gbM, * 13 nESO 92-8
NGC 3136 A10 03 33.0-67 26 56IBm15.615.02 × 0.3pB, pS, R, gbM, * 13 nESO 92-7, FGCE 794, AM 1002-671
NGC 3136 B10 10 13.2-67 00 18E412.711.71.4 × 0.8pB, pS, R, gbM, * 13 nESO 92-13, AM 1007-664
IC 220007 28 17.4-62 21 10Sb/P14.113.21.2 × 0.7eF, eS, eE 65°, bet 2 st, suspESO 123-12, AM 0727-621, IRAS 07276-6214
IC 2200 A07 28 06.6-62 21 47E/SB013.712.71.3 × 0.9eF, eS, eE 65°, bet 2 st, suspESO 123-11, AM 0727-621
IC 2554 A10 08 50.5-67 01 54SBbc12.511.83 × 1.2cF, S, cE 10°, N, spirESO 92-12, IRAS 10075-6647
IC 2554 B10 08 51.6-67 01 17SBc14.013.32 × 1cF, S, cE 10°, N, spirESO 92-12A
IC 259610 34 12.2-73 14 24SBab14.613.81.2 × 0.8eF, pS, bMESO 38-2, FAIR 283, IRAS 10329-7258

«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 G264.4-12.707 47 21-51 15 11He 2- 5264-12.107460-5107HENIZE 1964ESO 209-01, Sa 2- 17, StWr 3- 4, Wray 16- 8 3. 10. (O-III)AG82 91B: 14.65, V: 14.74Of(H)
PN G278.1-05.909 21 26-58 18 48NGC 2867278-05.109200-5805HERSCHEL 1834ARO 509, ESO 126-08, He 2- 27, StWr 3- 6, VV 52, VV' 89, Wray 16- 43 14. 1.3 +12.0 ± 4.0 18.9 (O-III), 23.5 (N-II)AG82 117, CSI -58 -09200, HD 81119B: 16.62WC 3
PN G278.5-04.509 30 56-57 36 58He 2- 32278-04.109294-5723HENIZE 1964ESO 166-19, Sa 3- 9, Wray 16- 49 35.
PN G278.6-06.709 19 28-59 12 07He 2- 26278-06.109181-5859HENIZE 1964ESO 126-06, My 47, Sa 2- 41, StWr 3- 5, Wray 16- 41 0.
PN G281.0-05.609 38 48-60 05 28IC 2501281-05.109373-5951FLEMING 1904ARO 510, He 2- 33, Sa 2- 47, StWr 3- 7, VV 53, VV'92, Wray 16- 54 2. 1.7 +32.7 ± 1.0AG82 119, CD -59 2483, HD 83832B: 14.42, V: 14.48
PN G283.8-04.210 03 50-60 43 47He 2- 39283-04.110022-6029HENIZE 1964ESO 127-03, Sa 2- 52, Wray 16- 64 10.4 -23.0 ± 20.0B: 17.9, V: 16.4
PN G283.9-01.810 15 34-58 51 10Hf 4283-01.110138-5836HOFFLEIT 1953ESO 127-12, He 2- 45, Sa 3- 12, Wray 16- 69 21. +22.0 ± 12.0< 10.0 (O-III)AG82 126
PN G285.4-01.110 28 43-59 04 10Pe 2- 5285-01.1PEREK 1960ESO 127-22, VV' 99 90. :
PN G285.4-05.310 09 22-62 36 41IC 2553285-05.110077-6222FLEMING 1893ESO 127-10, He 2- 42, Sa 2- 55, VV 55, VV' 95, Wray 16- 67 9. +37.3 ± 6.3AG82 125, CSI -62 -10077, HD 88367B: 15.4, V: 15.5
PN G285.6-02.710 23 09-60 32 35He 2- 47285-02.110214-6017HENIZE 1964ESO 127-16, My 59, SaSt 2- 5, Wray 15- 558< 5. B: 13.32, V: 12.98
PN G285.7-14.909 07 06-69 56 17IC 2448285-14.109066-6944FLEMING 1898ARO 506, ESO 061-01, He 2- 19, Sa 2- 34, StWr 3- 8, VV 49, VV'84, Wray 16- 34 9. 3.5 -24.0 ± 4.0 11.5 (O-III), 13.5 (N-II)AG82 111, CSI -69 -09066, HD 78991B: 13.97, V: 14.22O(H)
PN G286.0-06.510 07 23-63 54 32He 2- 41286-06.110059-6339HENIZE 1964ESO 092-11, Sa 2- 54, Wray 16- 66 0.
PN G286.2-06.910 06 56-64 21 46Wray 17- 4010055-6407WRAY 1966 60. : B: 16.97, V: 16.97
PN G286.3-04.810 17 50-62 40 09NGC 3211286-04.110162-6225HERSCHEL 1837ARO 512, ESO 127-15, He 2-46, Sa 2- 59, VV 56, VV' 97, Wray 16- 70 16. 2.5 -22.0 ± 2.0 26.5 (O-III), 31.0 (N-II)AG82 126bis, CSI -62 -10162, HD 89516B: 18.00
PN G288.4+00.310 54 35-59 09 48Hf 38288+00.110525-5853HOFFLEIT 1953ESO 128-19, He 2- 56, Sa 2-69, Wray 16- 80 25. +64.0 ± 4.0< 6.0 (O-III)
PN G288.4-02.410 44 31-61 39 41Pe 1- 3288-02.1PEREK 1960ESO 128-09, He 2- 54, Sa 2- 67, VV'104, Wray 16- 78 8.
PN G288.8-05.210 35 46-64 19 04He 2- 51288-05.110340-6403HENIZE 1964ESO 092-23, Sa 2- 63, Wray 16- 74 9.1 +8.0 ± 3.0< 10.0 (O-III)B: 17.15, V: 15.66
PN G288.9-00.810 53 59-60 26 42Hf 39288-00.110520-6010HOFFLEIT 1953ESO 128-18, He 3-519, Wray 15-682 72. AG82 131, CPD - 59 2824, HD 305696, SS73 25B: 12.53, V: 11.16Be pec., Sa 76
PN G289.6-01.610 56 03-61 28 02He 2- 57289-01.1HENIZE 1964ESO 128-20, Sa 3- 13 20.
PN G290.1-00.411 03 56-60 36 05Hf 48290-00.1HOFFLEIT 1953ESO 128-29, He 2- 60, Sa 2- 71, Wray 16- 85 19.
PN G291.6-04.811 00 20-65 14 54IC 2621291-04.110583-6458FLEMING 1907ARO 513, ESO 093-04, He 2- 59, Sa 2- 70, VV 58, VV' 105, Wray 16- 81 5. +13.6 ± 6.6AG82 133, CSI -64 -10584, HD 95541B: 16.4, V: 15.4
PN G295.3-09.311 17 43-70 49 30He 2- 62295-09.111157-7033HENIZE 1964Sa 2- 72, StWr 1- 4, Wray 16- 86 0.

«A Catalog of Parameters for Globular Clusters in the Milky Way» William E. Harris, 1996 [148]
IDNameRADecRSun
[kpc]
RGC
[kpc]
Fe/HwtEB-VVHB(m-M)VVtMV,tU-BB-VV-RV-Isptellipvr
[km/s]
vLSR
[km/s]
sigv
[km/s]
crc
[']
rh
[']
μVρ0lg(tc)lg(th)
NGC 280809 12 03.10-64 51 48.69.611.1-1.1440.2216.2215.596.20-9.390.280.920.571.18F70.12101.6 ± 0.789.213.4 ± 1.21.56 0.250.8015.084.668.249.15

Quellenangaben

7«Der grosse Kosmos-Himmelsführer» von Ian Ridpath und Wil Tirion; Kosmos Verlag; ISBN 3-440-05787-9
9«Drehbare Sternkarte SIRIUS» von H. Suter-Haug; Hallwag-Verlag, Bern
15«Hartung's Astronomical Objects for Southern Telescopes» by David Malin and David J. Frew; Melbourne University Press 1995; ISBN 0-522-84553-3
28«Uranometria omnium asterismorum continens schemata, nova methodo delineata aereis laminis expressa» Johann Bayer, Augsburg, 1603; DOI:10.3931/e-rara-309
87The Starry Sky: Canopus and Carina the Keel by Deborah Byrd; Astronomy 2/96, p.64
141Strasbourg-ESO Catalogue of Galactic Planetary Nebulae; A. Acker, F. Ochsenbein, B. Stenholm, R. Tylenda, J. Marcout, C. Schohn; European Southern Observatory; ISBN 3-923524-41-2 (1992); Bibcode:1992secg.book.....A; cdsarc.u-strasbg.fr/viz-bin/cat/V/84
148«A Catalog of Parameters for Globular Clusters in the Milky Way» Harris, William E.; Astronomical Journal v.112, p.1487, October 1996 / Revision: December 2010; DOI:10.1086/118116; Bibcode:1996AJ....112.1487H; physwww.mcmaster.ca/~harris/mwgc.dat (2021-01-03)
150IAU: The Constellations, 11. Oktober 2020; iau.org/public/themes/constellations
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277«Historische Deep-Sky Kataloge» von Dr. Wolfgang Steinicke; klima-luft.de/steinicke (2021-02-17)