This constellation's Bayer designations (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis. After Argo Navis was broken up into Carina, Vela, and Puppis, these Greek-letter designations were kept, so that Carina does not have a full complement of Greek-letter designations. For example, since Argo Navis's gamma star went to Vela, there is no Gamma Carinae.
| Name | B | Var | HD | HIP | RA | Dec | vis.
mag. | abs.
mag. | Dist. (ly) | Sp. class | Notes |
|---|
| Canopus | α | 45348 | 30438 | 06|23|57.09}} | −52|41|44.6}} | −0.72 | −5.53 | 313 | F0Ib | Suhel;[1] 2nd brightest star, nearest supergiant |
| β Car | β | 80007 | 45238 | 09|13|12.24}} | −69|43|02.9}} | 1.67 | −0.99 | 111 | A2IV | Miaplacidus |
| ε Car | ε | 71129 | 41037 | 08|22|30.86}} | −59|30|34.3}} | 1.86 | −4.58 | 632 | K3III+B2V | Avior; suspected eclipsing binary, {{Variable star|1.82|1.94}} |
| ι Car | ι | 80404 | 45556 | 09|17|05.43}} | −59|16|30.9}} | 2.23 | −4.43 | 692 | A8Ib | Aspidiske, Turais, Scutulum; suspected variable, {{Variable star|2.23|2.28}} |
| θ Car | θ | 93030 | 52419 | 10|42|57.43}} | −64|23|40.1}} | 2.74 | −2.91 | 439 | B0Vp | in IC 2602 |
| υ Car | υ | 85123 | 48002 | 09|47|06.14}} | −65|04|19.3}} | 2.92 | −5.56 | 1622 | A9 | binary star |
| ω Car | ω | 89080 | 50099 | 10|13|44.28}} | −70|02|16.5}} | 3.29 | −1.99 | 370 | B8III |
| p Car | p | PP | 91465 | 51576 | 10|32|01.48}} | −61|41|07.3}} | 3.30 | −2.62 | 497 | B4Vne | γ Cas variable, {{Variable star|3.22|3.55}} |
| V337 Car | q | V337 | 89388 | 50371 | 10|17|05.01}} | −61|19|56.4}} | 3.39 | −3.38 | 736 | K3II | irregular variable, {{Variable star|3.36|3.44}} |
| a Car | a | V357 | 79351 | 45080 | 09|10|58.11}} | −58|58|00.9}} | 3.43 | −2.11 | 418 | B2IV | eclipsing binary, {{Variable star|3.41|3.44}} |
| χ Car | χ | 65575 | 38827 | 07|56|46.74}} | −52|58|56.6}} | 3.46 | −1.91 | 387 | B3IVp | β Cep variable, {{VSA|0.015|0.10}} |
| l Car | l | 84810 | 47854 | 09|45|14.83}} | −62|30|28.5}} | 3.69 | −4.64 | 1509 | G5Iab/Ib | classical Cepheid, {{Variable star|3.28|4.18|35.54}} |
| HD 94510 | u | 94510 | 53253 | 10|53|29.57}} | −58|51|11.8}} | 3.78 | 1.42 | 97 | K0III-IV... | suspected variable, {{Variable star|3.75|3.80}} |
| HD 90853 | s | 90853 | 51232 | 10|27|52.75}} | −58|44|21.9}} | 3.81 | −3.71 | 1042 | F2II | suspected variable |
| HD 76728 | c | 76728 | 43783 | 08|55|02.86}} | −60|38|41.0}} | 3.84 | −1.06 | 312 | B8III | double star |
| V382 Car | x | V382 | 96918 | 54463 | 11|08|35.40}} | −58|58|30.2}} | 3.93 | −7.37 | 5927 | G0Ia0 | hypergiant; slow irregular variable, {{Variable star|3.77|4.05}} |
| HD 79447 | i | 79447 | 45101 | 09|11|16.77}} | −62|19|01.3}} | 3.96 | −1.97 | 499 | B3IV | 0.008|22.26}} |
| HD 90589 | I | 90589 | 50954 | 10|24|23.74}} | −74|01|53.6}} | 3.99 | 2.94 | 53 | F2IV | 3.96|4.00}} |
| HD 83183 | h | 83183 | 46974 | 09|34|26.66}} | −59|13|47.2}} | 4.08 | −4.83 | 1976 | B5II |
| V343 Car | d | V343 | 74375 | 42568 | 08|40|37.04}} | −59|45|39.7}} | 4.31 | −3.87 | 1411 | B1.5III | β Cep variable |
| HD 80230 | g | 80230 | 45496 | 09|16|12.10}} | −57|32|29.2}} | 4.34 | −1.74 | 536 | M1III | 4.31|4.35}} |
| HD 47306 | N | 47306 | 31407 | 06|34|58.59}} | −52|58|32.3}} | 4.35 | −4.31 | 1762 | B9III |
| HR 2554 | A | V415 | 50337 | 32761 | 06|49|51.32}} | −53|37|21.0}} | 4.39 | −1.74 | 553 | G6II | Algol variable, {{VSA|0.06}} |
| HD 91942 | r | 91942 | 51849 | 10|35|35.31}} | −57|33|27.5}} | 4.45 | −3.68 | 1376 | K3/K4II | suspected variable |
| η Car | η | 93308 | 10|45|03.60}} | −59|41|03.0}} | 4.47 | 7500 | LBV | in Trumpler 16; binary star; luminous blue variable, {{Variable star|−0.8|7.9}}; surrounded by the Homunculus Nebula; one of the most luminous and most massive stars known. |
| HR 3643 | G | 78791 | 44599 | 09|05|08.83}} | −72|36|09.7}} | 4.47 | −1.25 | 454 | F6II-III |
| V344 Car | f | V344 | 75311 | 43105 | 08|46|42.56}} | −56|46|11.3}} | 4.50 | −1.62 | 546 | B3Vne | γ Cas variable, {{Variable star|4.40|4.51}} |
| HD 83944 | m | 83944 | 47391 | 09|39|21.04}} | −61|19|41.2}} | 4.51 | 0.33 | 224 | B9V | suspected variable |
| V520 Car | w | V520 | 93070 | 52468 | 10|43|32.31}} | −60|33|59.9}} | 4.58 | −2.99 | 1065 | K3Ib | irregular variable, {{Variable star|4.50|4.59}} |
| V533 Car | y | V533 | 97534 | 54751 | 11|12|36.02}} | −60|19|03.5}} | 4.59 | −8.34 | 12538 | A6Ia | α Cyg variable |
| HD 96566 | z1 | 96566 | 54301 | 11|06|32.47}} | −62|25|26.9}} | 4.62 | −0.65 | 370 | G8III |
| V399 Car | P | V399 | 90772 | 51192 | 10|27|24.48}} | −57|38|19.7}} | 4.65 | A6Ia | semiregular variable, {{Variable star|4.63|4.72|88.3}} |
| V345 Car | E | V345 | 78764 | 44626 | 09|05|38.38}} | −70|32|18.7}} | 4.67 | −2.94 | 1079 | B2IVe | γ Cas variable, {{Variable star|4.67|4.78|137.7}} |
| HD 92397 | t2 | 92397 | 52102 | 10|38|45.01}} | −59|10|58.8}} | 4.69 | −4.08 | 1852 | K4/K5III: | suspected variable |
| HD 91375 | K | 91375 | 51438 | 10|30|20.08}} | −71|59|33.8}} | 4.72 | 0.22 | 259 | A2III |
| HR 3220 | B | 68456 | 39903 | 08|09|00.86}} | −61|18|06.1}} | 4.74 | 3.09 | 70 | F5V |
| V518 Car | V518 | 92938 | 52370 | 10|42|14.14}} | −64|27|59.2}} | 4.76 | −0.97 | 456 | B3V | in IC 2602; γ Cas variable |
| HD 81101 | k | 81101 | 45856 | 09|20|56.83}} | −62|24|16.7}} | 4.79 | 0.62 | 223 | G6III |
| HD 93194 | 93194 | 52502 | 10|44|06.94}} | −63|57|40.0}} | 4.80 | −1.06 | 484 | B5Vn | in IC 2602; suspected irregular variable, {{Variable star|4.79|4.84}} |
| HD 66591 | D | 66591 | 39138 | 08|00|19.97}} | −63|34|03.0}} | 4.81 | −1.29 | 542 | B3V | suspected variable |
| HD 73389 | e2 | 73389 | 42134 | 08|35|19.65}} | −58|00|33.5}} | 4.84 | 0.60 | 229 | K0III |
| HD 93607 | 93607 | 52736 | 10|46|51.24}} | −64|23|00.6}} | 4.87 | −0.83 | 449 | B3IV | in IC 2602; suspected variable |
| HD 61248 | Q | 61248 | 36942 | 07|35|39.70}} | −52|32|01.7}} | 4.93 | −0.48 | 394 | K3III | suspected variable |
| V376 Car | b1 | V376 | 77002 | 43937 | 08|56|58.43}} | −59|13|45.7}} | 4.93 | −1.47 | 621 | B2IV-V | β Cep variable, {{Variable star|4.91|4.96|0.021}} |
| HD 91496 | 91496 | 51495 | 10|31|02.07}} | −73|13|17.4}} | 4.94 | −2.42 | 964 | K4/K5III | suspected variable, {{Variable star|4.87|4.97}} |
| HD 90264 | L | 90264 | 50847 | 10|22|58.18}} | −66|54|05.5}} | 4.97 | −0.63 | 430 | B8V |
| HD 92063 | t1 | 92063 | 51912 | 10|36|20.56}} | −59|33|51.5}} | 5.08 | 0.50 | 269 | K1III |
| HD 59219 | 59219 | 36114 | 07|26|21.86}} | −51|01|06.6}} | 5.09 | −1.09 | 562 | K0III |
| HD 96919 | z2 | V371 | 96919 | 54461 | 11|08|34.01}} | −61|56|49.8}} | 5.12 | −6.03 | 5525 | B9Ia | α Cyg variable, {{Variable star|5.12|5.19}} |
| HD 53047 | 53047 | 33779 | 07|00|51.51}} | −51|24|09.5}} | 5.14 | −1.25 | 617 | M1III | semiregular variable |
| V386 Car | V386 | 54118 | 34105 | 07|04|18.32}} | −56|44|59.0}} | 5.14 | 0.45 | 282 | A0p: | α2 CVn variable, {{VSA|0.026|3.28}} |
| HD 88981 | M | 88981 | 50083 | 10|13|30.68}} | −66|22|22.2}} | 5.15 | 0.31 | 304 | Am |
| HD 69863 | C | 69863 | 40429 | 08|15|15.95}} | −62|54|56.2}} | 5.16 | 0.81 | 242 | A+... | binary star |
| HD 77370 | b2 | 77370 | 44143 | 08|59|24.38}} | −59|05|03.8}} | 5.17 | 3.08 | 85 | F3V |
| HR 3153 | V460 | 66342 | 39070 | 07|59|37.55}} | −60|35|13.5}} | 5.19 | −2.34 | 1045 | M0II | in NGC 2516; semiregular variable, {{Variable star|5.15|5.3}} |
| HD 97583 | 97583 | 54767 | 11|12|45.27}} | −64|10|11.2}} | 5.22 | 0.30 | 314 | B9V | double star |
| HD 93549 | 93549 | 52701 | 10|46|29.61}} | −64|15|47.7}} | 5.23 | −0.37 | 429 | B7IV | in IC 2602 |
| HD 88323 | 88323 | 49698 | 10|08|42.84}} | −65|48|55.9}} | 5.26 | 0.16 | 341 | K0III | optical double |
| V524 Car | V524 | 94367 | 53154 | 10|52|30.85}} | −57|14|25.5}} | 5.26 | −6.08 | 6037 | B9Ia | α Cyg variable |
| HD 73390 | e1 | 73390 | 42129 | 08|35|15.58}} | −58|13|29.1}} | 5.27 | −2.08 | 962 | B3V+... |
| HD 91056 | 91056 | 51313 | 10|28|52.60}} | −64|10|20.2}} | 5.27 | −4.64 | 3135 | K3Ib | slow irregular variable |
| HD 80951 | 80951 | 45581 | 09|17|25.21}} | −74|53|39.8}} | 5.28 | −1.44 | 721 | A1V |
| HD 84121 | 84121 | 47479 | 09|40|42.60}} | −57|59|00.9}} | 5.30 | 1.16 | 220 | A3IV |
| HD 93540 | 93540 | 52678 | 10|46|16.58}} | −64|30|52.5}} | 5.33 | −0.45 | 466 | B7:V | in IC 2602; suspected variable |
| HD 92964 | V519 | 92964 | 52405 | 10|42|40.57}} | −59|12|56.8}} | 5.36 | −6.23 | 6792 | B2.5Ia | α Cyg variable, {{Variable star|5.32|5.43|14.68}} |
| HD 57917 | 57917 | 35589 | 07|20|38.81}} | −52|05|09.3}} | 5.38 | −0.52 | 493 | B9V |
| HD 80671 | 80671 | 45571 | 09|17|17.40}} | −68|41|22.5}} | 5.38 | 2.75 | 109 | F4V |
| HD 49689 | 49689 | 32494 | 06|46|52.69}} | −51|15|55.6}} | 5.39 | −1.83 | 906 | K1II/IIIp+G: | suspected variable |
| HD 73887 | 73887 | 42286 | 08|37|18.85}} | −62|51|12.3}} | 5.45 | 0.39 | 335 | K0III |
| HD 82350 | 82350 | 46358 | 09|27|06.50}} | −71|36|07.5}} | 5.46 | 1.51 | 201 | K2III |
| HD 83095 | H | 83095 | 46741 | 09|31|36.32}} | −73|04|51.3}} | 5.46 | −1.47 | 791 | K4III |
| HD 92207 | V370 | 92207 | 52004 | 10|37|27.08}} | −58|44|00.0}} | 5.47 | −6.52 | 8150 | A0Ia | α Cyg variable, {{Variable star|5.45|5.52|1.33}} |
| V450 Car | V450 | 53921 | 34000 | 07|03|15.11}} | −59|10|41.3}} | 5.50 | −0.35 | 482 | B9IV | 0.02}} |
| HD 92664 | V364 | 92664 | 52221 | 10|40|11.46}} | −65|06|00.9}} | 5.51 | −0.26 | 466 | B9p Si | α2 CVn variable, {{Variable star|5.48|5.52|1.67}} |
| HD 67364 | 67364 | 39566 | 08|05|03.71}} | −53|06|28.5}} | 5.52 | 0.11 | 393 | K3/K4III |
| HD 79698 | 79698 | 45219 | 09|12|55.62}} | −59|24|50.3}} | 5.54 | −0.28 | 475 | G6II |
| HD 85656 | 85656 | 48310 | 09|50|55.60}} | −62|44|42.5}} | 5.56 | −1.78 | 959 | K1IIICN... |
| HD 64067 | 64067 | 38152 | 07|49|06.72}} | −56|24|37.4}} | 5.57 | −1.72 | 934 | G5II |
| HD 46569 | 46569 | 31079 | 06|31|18.22}} | −51|49|34.3}} | 5.58 | 2.73 | 121 | F8V |
| HD 96706 | 96706 | 54327 | 11|06|49.93}} | −70|52|40.6}} | 5.58 | −2.12 | 1128 | B2V | 0.004|1.74}} |
| HD 65907 | 65907 | 38908 | 07|57|46.30}} | −60|18|12.1}} | 5.59 | 4.54 | 53 | G2V... |
| HD 76113 | 76113 | 43499 | 08|51|36.53}} | −57|38|01.0}} | 5.59 | −1.12 | 716 | B8III |
| V448 Car | O | V448 | 49877 | 32531 | 06|47|18.71}} | −55|32|24.2}} | 5.60 | −0.72 | 598 | K5III | semiregular variable |
| HD 65273 | 65273 | 38656 | 07|54|53.39}} | −57|18|10.4}} | 5.62 | 0.51 | 343 | K3/K4III |
| HD 68434 | 68434 | 39957 | 08|09|33.63}} | −56|05|07.7}} | 5.66 | 0.33 | 380 | A3m... |
| HD 89715 | 89715 | 50520 | 10|19|05.12}} | −64|40|34.6}} | 5.66 | 0.90 | 292 | A1V |
| V372 Car | V372 | 64722 | 38438 | 07|52|29.75}} | −54|22|01.9}} | 5.69 | −2.56 | 1462 | B1.5IV | β Cep variable, {{VSA|0.027|0.12}} |
| HD 88661 | QY | 88661 | 49934 | 10|11|46.47}} | −58|03|38.0}} | 5.70 | −2.29 | 1294 | B2IVnpe | γ Cas variable, {{Variable star|5.63|5.83}} |
| S Car | S | 88366 | 49751 | 10|09|22.01}} | −61|32|57.1}} | 5.71 | 1780 | K5-M6e | Mira variable, {{Variable star|4.5|9.9|149.49}} |
| HD 97670 | 97670 | 54829 | 11|13|30.79}} | −59|37|09.5}} | 5.73 | −3.00 | 1821 | B1.5V | suspected variable |
| HD 65662 | 65662 | 38783 | 07|56|18.65}} | −60|31|35.3}} | 5.74 | −2.17 | 1244 | K4II | in NGC 2516 |
| HD 93163 | 93163 | 52487 | 10|43|51.21}} | −64|14|56.6}} | 5.75 | −1.71 | 1009 | B3:V | 0.03}} |
| HD 66194 | V374 | 66194 | 38994 | 07|58|50.56}} | −60|49|28.2}} | 5.77 | −1.72 | 1028 | B2IVnpe | in NGC 2516; γ Cas variable, {{Variable star|5.72|5.84}} |
| HD 81830 | 81830 | 46225 | 09|25|27.38}} | −61|57|02.2}} | 5.77 | 1.47 | 236 | A4V+... |
| HD 64185 | 64185 | 38160 | 07|49|12.95}} | −60|17|02.5}} | 5.78 | 3.06 | 114 | F1V | spectroscopic binary |
| HD 76538 | 76538 | 43669 | 08|53|48.67}} | −60|21|14.2}} | 5.78 | −2.35 | 1376 | B5III |
| HD 85655 | 85655 | 48339 | 09|51|12.03}} | −59|25|32.4}} | 5.79 | −1.01 | 746 | K2IIICNp... |
| HD 77615 | 77615 | 44256 | 09|00|45.75}} | −60|57|49.8}} | 5.80 | −2.13 | 1259 | G8II |
| HD 84152 | 84152 | 47498 | 09|41|02.10}} | −57|15|34.0}} | 5.80 | 0.57 | 362 | K0/K1III |
| HD 88473 | 88473 | 49764 | 10|09|30.20}} | −68|40|58.2}} | 5.80 | −0.46 | 583 | A0IV |
| HD 49517 | 49517 | 32402 | 06|45|53.72}} | −52|24|35.0}} | 5.81 | −2.32 | 1376 | K3III |
| HD 93943 | 93943 | 52922 | 10|49|24.46}} | −59|19|25.6}} | 5.85 | −1.24 | 853 | B9.5IV/V |
| HD 80950 | 80950 | 45585 | 09|17|27.63}} | −74|44|04.8}} | 5.86 | 1.32 | 264 | A0V |
| HD 60060 | 60060 | 36444 | 07|29|59.74}} | −52|39|04.6}} | 5.87 | 0.84 | 330 | K0III |
| HD 66441 | 66441 | 39184 | 08|00|49.96}} | −54|09|04.7}} | 5.87 | −0.79 | 700 | B5Vn | suspected variable |
| V482 Car | V482 | 82536 | 46620 | 09|30|23.45}} | −58|21|42.9}} | 5.88 | −1.68 | 1058 | M2III | semiregular variable |
| V514 Car | V514 | 92287 | 52043 | 10|38|02.66}} | −57|15|22.7}} | 5.89 | −2.08 | 1278 | B3IV | 5.88|5.92|2.90}} |
| HD 82406 | 82406 | 46460 | 09|28|30.60}} | −66|42|07.2}} | 5.90 | 1.33 | 268 | A0V |
| HD 82347 | 82347 | 46482 | 09|28|47.19}} | −62|16|23.5}} | 5.91 | 0.06 | 482 | K1III |
| HD 87283 | 87283 | 49164 | 10|02|00.11}} | −60|25|15.2}} | 5.93 | −4.03 | 3196 | A9IV | possibly in NGC 3114 |
| HD 90454 | 90454 | 50993 | 10|24|59.50}} | −58|34|34.7}} | 5.93 | 1.13 | 297 | F2III |
| T Car | T | 94776 | 53394 | 10|55|17.26}} | −60|31|01.9}} | 5.93 | 1.07 | 306 | K0III | not variable |
| HD 60228 | 60228 | 36496 | 07|30|30.91}} | −54|23|58.0}} | 5.95 | 0.33 | 433 | M1III |
| HD 94683 | 94683 | 53334 | 10|54|29.60}} | −61|49|35.8}} | 5.95 | −2.59 | 1663 | K4III | suspected variable |
| HD 54732 | 54732 | 34349 | 07|07|13.30}} | −51|58|06.2}} | 5.96 | −0.23 | 564 | K0III |
| HD 56705 | 56705 | 35084 | 07|15|21.27}} | −52|29|58.3}} | 5.96 | 0.58 | 389 | K0V |
| HD 70839 | 70839 | 40932 | 08|21|12.10}} | −57|58|23.6}} | 5.96 | −3.36 | 2380 | B1.5III |
| HD 92436 | 92436 | 52127 | 10|38|59.70}} | −58|49|00.8}} | 5.96 | −0.53 | 648 | M1III |
| HD 91533 | 91533 | 51623 | 10|32|47.82}} | −58|40|00.3}} | 5.98 | −6.71 | 11241 | A2Iab | suspected variable |
| V522 Car | V522 | 93737 | 52827 | 10|48|05.42}} | −59|55|09.0}} | 5.98 | A0Ia | α Cyg variable |
| HD 81613 | 81613 | 46101 | 09|24|05.50}} | −61|38|55.6}} | 5.99 | 0.92 | 337 | K0III |
| HD 94650 | 94650 | 53272 | 10|53|42.13}} | −70|43|13.2}} | 5.99 | −0.89 | 776 | B6V |
| HD 98560 | 98560 | 55280 | 11|19|16.84}} | −64|34|57.4}} | 5.99 | 3.12 | 122 | F6IV |
| HD 90874 | 90874 | 51194 | 10|27|25.40}} | −65|42|17.0}} | 6.00 | 1.76 | 229 | A2V |
| HD 53349 | 53349 | 33800 | 07|01|05.18}} | −58|56|25.1}} | 6.01 | 2.36 | 175 | F0V | suspected variable |
| HD 76346 | 76346 | 43620 | 08|53|03.80}} | −56|38|58.5}} | 6.02 | 1.23 | 296 | A0V | has a planet (b) |
| HD 80094 | 80094 | 45418 | 09|15|17.66}} | −58|23|18.2}} | 6.02 | 0.00 | 522 | B7IV | 0.008|1.56}} |
| HD 56239 | 56239 | 34780 | 07|12|01.98}} | −63|11|24.2}} | 6.03 | −0.29 | 598 | A0IV/V |
| HD 57852 | 57852 | 35564 | 07|20|21.46}} | −52|18|42.8}} | 6.05 | 113 | F5V | component of the HIP 35564 system; suspected variable |
| HD 82068 | 82068 | 46328 | 09|26|44.18}} | −64|55|47.5}} | 6.05 | 1.88 | 223 | A3Vn |
| V390 Car | V390 | 61966 | 37248 | 07|39|00.34}} | −53|16|24.2}} | 6.06 | −0.05 | 544 | B9IV-Vp... | α2 CVn variable, {{VSA|0.004}} |
| V535 Car | V535 | 98292 | 55140 | 11|17|19.02}} | −67|49|24.6}} | 6.06 | −2.52 | 1698 | M2III | slow irregular variable |
| HD 88825 | 88825 | 50044 | 10|13|01.16}} | −59|55|05.1}} | 6.07 | −2.84 | 1976 | B4Ve |
| HD 96544 | 96544 | 54294 | 11|06|29.30}} | −58|40|30.1}} | 6.07 | −1.81 | 1226 | K2II/III |
| HD 92682 | 92682 | 52150 | 10|39|15.94}} | −74|29|36.2}} | 6.08 | −1.57 | 1105 | K3II | 0.005|0.084}} |
| HD 63382 | 63382 | 37854 | 07|45|35.52}} | −56|43|21.3}} | 6.10 | −1.20 | 942 | F0II |
| R Car | R | 82901 | 46806 | 09|32|14.60}} | −62|47|20.0}} | 6.10 | 416 | M6.5 IIIpev | Mira variable, {{Variable star|3.9|10.5|308.71}} |
| HD 91619 | V369 | 91619 | 51676 | 10|33|25.40}} | −58|11|24.6}} | 6.11 | −6.99 | 13583 | B7Ia | α Cyg variable, {{VSA|0.1|1.12}} |
| U Car | U | 95109 | 53589 | 10|57|48.19}} | −59|43|55.9}} | 6.11 | G3Ia | classical Cepheid, {{Variable star|5.74|6.96|38.83}} |
| HD 70982 | 70982 | 40926 | 08|21|07.65}} | −64|06|21.4}} | 6.11 | 0.34 | 464 | G6/G8III |
| V461 Car | V461 | 66546 | 39225 | 08|01|23.05}} | −54|30|56.0}} | 6.12 | −1.92 | 1320 | B2IV-V | Algol variable |
| HD 65908 | 65908 | 38863 | 07|57|12.76}} | −63|17|48.8}} | 6.14 | 0.37 | 464 | B8V |
| V478 Car | V478 | 80710 | 45615 | 09|17|51.67}} | −67|03|03.2}} | 6.14 | −1.96 | 1358 | K2III | semiregular variable |
| HD 87543 | 87543 | 49281 | 10|03|34.14}} | −61|53|02.6}} | 6.14 | −2.49 | 1734 | B4:Vne |
| HD 95208 | 95208 | 53546 | 10|57|15.81}} | −75|05|59.2}} | 6.16 | −3.12 | 2345 | K1II |
| HD 95324 | 95324 | 53701 | 10|59|14.05}} | −61|19|14.7}} | 6.16 | 0.93 | 363 | B8IV |
| HD 96088 | 96088 | 54082 | 11|04|00.25}} | −57|57|19.2}} | 6.16 | −3.63 | 2964 | B3III |
| HD 47001 | 47001 | 31265 | 06|33|26.31}} | −52|19|45.5}} | 6.18 | −0.17 | 607 | G8III |
| V492 Car | V492 | 86659 | 48782 | 09|56|59.84}} | −69|06|06.6}} | 6.18 | −1.43 | 1087 | B3V | 53 Per variable |
| HD 87436 | 87436 | 49233 | 10|02|59.95}} | −60|10|43.3}} | 6.18 | −3.80 | 3228 | A6II/III | suspected variable |
| HD 90630 | 90630 | 50976 | 10|24|44.56}} | −73|58|18.3}} | 6.18 | 0.53 | 441 | A2/A3V | suspected variable |
| V655 Car | V655 | 91272 | 51425 | 10|30|08.81}} | −66|59|04.8}} | 6.19 | −1.70 | 1235 | B4IV | Algol variable, {{Variable star|6.19|6.36|16.93}} |
| HD 62897 | 62897 | 37599 | 07|42|53.36}} | −58|13|48.5}} | 6.20 | −0.23 | 629 | K0III |
| HD 75086 | 75086 | 42936 | 08|45|05.55}} | −58|43|27.6}} | 6.20 | −1.23 | 997 | B7III |
| HD 87238 | 87238 | 49160 | 10|01|58.09}} | −57|20|59.4}} | 6.20 | −0.62 | 753 | K1II |
| HD 84850 | 84850 | 47913 | 09|45|55.82}} | −58|47|38.4}} | 6.22 | 1.68 | 264 | F5IV |
| HD 89263 | 89263 | 50287 | 10|16|03.26}} | −59|54|12.4}} | 6.22 | 1.63 | 270 | A5V |
| V532 Car | V532 | 97451 | 54708 | 11|12|03.60}} | −58|25|24.1}} | 6.24 | −0.53 | 736 | M4III | semiregular variable |
| HD 91767 | 91767 | 51732 | 10|34|12.72}} | −60|59|15.5}} | 6.25 | −0.78 | 830 | K2/K3III | suspected variable |
| HD 65750 | V341 | 65750 | 38834 | 07|56|50.70}} | −59|07|35.0}} | 6.25 | 967 | M0III | 6.2|7.1}} |
| HD 93344 | 93344 | 52520 | 10|44|20.10}} | −70|51|35.0}} | 6.25 | 1.12 | 346 | A5IV/V |
| HD 52603 | 52603 | 33588 | 06|58|39.81}} | −55|43|44.1}} | 6.26 | 1.59 | 280 | K2III |
| HD 74622 | 74622 | 42717 | 08|42|20.90}} | −55|46|28.8}} | 6.26 | 1.23 | 331 | K2III |
| υ Car B | υ | 85124 | 09|47|06.70}} | −65|04|21.0}} | 6.26 | 1623 | A8 Ib | component of the υ Car system |
| HD 93372 | 93372 | 52535 | 10|44|27.25}} | −72|26|37.1}} | 6.26 | 3.74 | 104 | F6V |
| HD 93502 | 93502 | 52679 | 10|46|17.12}} | −60|36|10.4}} | 6.26 | 1.01 | 365 | A0IV |
| HD 94491 | 94491 | 53231 | 10|53|21.18}} | −58|53|36.5}} | 6.26 | −2.16 | 1575 | B5V |
| HD 82858 | 82858 | 46737 | 09|31|33.05}} | −66|43|08.6}} | 6.27 | −0.40 | 703 | K1III |
| HD 66607 | 66607 | 39238 | 08|01|31.58}} | −55|27|16.8}} | 6.28 | −0.28 | 668 | B4V |
| V375 Car | V375 | 67536 | 39530 | 08|04|42.94}} | −62|50|10.9}} | 6.29 | 1249 | B2.5Vn | β Cep variable, {{VSA|0.04|1.02}} |
| HD 61031 | 61031 | 36856 | 07|34|39.58}} | −51|28|28.3}} | 6.29 | −1.76 | 1331 | A1III/IV |
| HD 93662 | 93662 | 52797 | 10|47|38.41}} | −57|28|02.7}} | 6.29 | −3.35 | 2763 | M1II | 6.28|6.41}} |
| HD 94275 | 94275 | 53100 | 10|51|46.93}} | −57|16|20.3}} | 6.29 | −0.05 | 604 | A6III |
| HD 63926 | 63926 | 38087 | 07|48|19.51}} | −56|28|15.9}} | 6.30 | −2.91 | 2264 | K0III+... |
| HD 66341 | 66341 | 39073 | 07|59|40.09}} | −60|12|26.6}} | 6.30 | −1.81 | 1364 | B8III | in NGC 2516 |
| HD 81502 | 81502 | 46049 | 09|23|27.33}} | −60|18|08.4}} | 6.30 | −2.91 | 2264 | K1/K2II/III |
| HD 86606 | 86606 | 48715 | 09|56|09.76}} | −71|23|21.5}} | 6.30 | −2.69 | 2050 | B1Ib |
| HD 68423 | 68423 | 39843 | 08|08|24.65}} | −63|48|03.0}} | 6.32 | −0.58 | 782 | B6V | suspected variable |
| HD 80126 | 80126 | 45437 | 09|15|34.73}} | −57|34|39.9}} | 6.32 | −1.32 | 1098 | G8II |
| QZ Car | QZ | 93206 | 52526 | 10|44|22.92}} | −59|59|36.0}} | 6.32 | −3.23 | 2650 | B0Ib: | in Collinder 228; β Lyr variable, {{Variable star|6.16|6.49|6.00}} |
| HD 82458 | 82458 | 46407 | 09|27|49.19}} | −71|46|52.3}} | 6.33 | 2.57 | 184 | F3/F5V |
| V486 Car | V486 | 84416 | 47591 | 09|42|12.99}} | −66|54|53.4}} | 6.33 | 0.04 | 592 | A0V | β Lyr variable |
| HD 92536 | 92536 | 52160 | 10|39|22.85}} | −64|06|42.5}} | 6.33 | 0.49 | 479 | B8V | in IC 2602 |
| HD 74341 | 74341 | 42579 | 08|40|43.55}} | −57|32|43.9}} | 6.34 | 2.13 | 227 | A3V |
| HD 90074 | 90074 | 50785 | 10|22|10.48}} | −58|15|56.3}} | 6.34 | 1.23 | 343 | G6III |
| HD 90289 | 90289 | 50916 | 10|23|50.66}} | −57|57|14.1}} | 6.34 | −0.59 | 793 | K5Ib-II | 6.33|6.35}} |
| HD 93649 | 93649 | 52730 | 10|46|48.09}} | −69|12|35.3}} | 6.34 | −2.04 | 1545 | A2IV |
| HD 97472 | 97472 | 54673 | 11|11|29.57}} | −71|26|10.3}} | 6.34 | 0.08 | 583 | K2/K3III |
| HD 74148 | 74148 | 42440 | 08|39|13.24}} | −60|19|02.4}} | 6.35 | 0.71 | 437 | A0V |
| HD 89805 | 89805 | 50562 | 10|19|42.04}} | −65|08|14.1}} | 6.35 | −2.59 | 2000 | K2II |
| WR 22 | V429 | 92740 | 52308 | 10|41|17.52}} | −59|40|36.9}} | 6.35 | −4.72 | 5344 | WN7 + A(SB1) | Wolf–Rayet star and Algol variable, {{Variable star|6.33|6.52|80.34}}; one of the most luminous stars known |
| HD 93739 | 93739 | 52785 | 10|47|30.62}} | −69|26|15.8}} | 6.35 | −1.57 | 1249 | B2IV |
| HD 65189 | 65189 | 38667 | 07|55|00.44}} | −52|35|00.1}} | 6.36 | −1.08 | 1003 | B8III |
| HD 72322 | 72322 | 41653 | 08|29|36.40}} | −55|11|27.3}} | 6.36 | −0.36 | 721 | G0V |
| V473 Car | V473 | 76640 | 43763 | 08|54|54.05}} | −58|14|22.9}} | 6.36 | −0.77 | 869 | B5V | 53 Per variable |
| HD 79699 | 79699 | 45214 | 09|12|50.63}} | −60|55|00.5}} | 6.36 | 0.21 | 553 | B9V |
| HD 78632 | 78632 | 44665 | 09|06|07.61}} | −64|29|59.7}} | 6.37 | 0.08 | 590 | K3III |
| HD 61394 | 61394 | 36977 | 07|36|01.62}} | −55|53|15.8}} | 6.39 | 0.06 | 601 | K1/K2IIICN. |
| HD 96568 | 96568 | 54289 | 11|06|24.32}} | −64|50|23.8}} | 6.39 | 0.58 | 473 | A3V |
| HD 44267 | 44267 | 29913 | 06|17|51.74}} | −52|43|58.9}} | 6.40 | −0.70 | 858 | K2/K3III | 0.008|1.32}} |
| HD 62758 | 62758 | 37530 | 07|42|10.22}} | −58|37|51.4}} | 6.40 | −1.18 | 1069 | B2.5V |
| V368 Car | V368 | 88647 | 49926 | 10|11|35.49}} | −58|49|40.2}} | 6.40 | 801 | M3III | 6.1|6.4}} |
| HD 51210 | 51210 | 33012 | 06|52|45.44}} | −59|20|28.6}} | 6.41 | 0.62 | 470 | A3m... |
| HD 87438 | 87438 | 49223 | 10|02|49.42}} | −62|09|24.0}} | 6.41 | −3.23 | 2763 | K3Ib | 6.38|6.43}} |
| HD 91270 | 91270 | 51461 | 10|30|39.24}} | −61|21|23.4}} | 6.41 | −0.57 | 811 | M2III | suspected variable |
| HD 84046 | 84046 | 47422 | 09|39|45.15}} | −62|56|34.7}} | 6.42 | 0.01 | 623 | B8/B9III/IVw... | 6.42|6.8}} |
| HD 88907 | 88907 | 50067 | 10|13|21.20}} | −61|39|31.8}} | 6.42 | −1.06 | 1022 | B2V |
| V507 Car | V507 | 90966 | 51265 | 10|28|18.28}} | −63|09|52.5}} | 6.42 | −2.56 | 2037 | B2/B3III:ne | Be star |
| HD 91094 | 91094 | 51327 | 10|29|03.67}} | −65|10|34.8}} | 6.42 | 0.00 | 627 | M1III | semiregular variable |
| HD 98025 | 98025 | 55003 | 11|15|42.76}} | −57|21|21.1}} | 6.42 | 0.16 | 583 | A3V |
| HD 78293 | 78293 | 44565 | 09|04|48.00}} | −57|51|09.5}} | 6.43 | −1.21 | 1101 | A8III |
| HD 93359 | 93359 | 52537 | 10|44|32.42}} | −70|51|18.9}} | 6.43 | 1.25 | 354 | A6IV |
| HD 65867 | 65867 | 38963 | 07|58|21.47}} | −51|26|54.9}} | 6.44 | 0.43 | 518 | A8/A9IV | suspected eclipsing binary |
| V469 Car | V469 | 72303 | 41644 | 08|29|29.82}} | −54|12|42.5}} | 6.44 | −0.28 | 720 | Ap Si | α2 CVn variable |
| HD 49705 | 49705 | 32477 | 06|46|41.70}} | −54|41|42.2}} | 6.45 | 0.93 | 414 | G6III |
| HD 81896 | 81896 | 46143 | 09|24|37.16}} | −70|04|32.8}} | 6.45 | 0.06 | 617 | K1III |
| V495 Car | V495 | 88158 | 49642 | 10|07|56.64}} | −62|13|17.2}} | 6.45 | −0.55 | 817 | Ap Si | α2 CVn variable |
| WR 24 | 93131 | 52488 | 10|43|52.27}} | −60|07|04.0}} | 6.46 | −5.05 | 6520 | WN7 + A | in Collinder 228; Wolf–Rayet star, {{Variable star|6.46|6.49|4.76}}; one of the most luminous stars known |
| HD 52622 | 52622 | 33577 | 06|58|36.39}} | −56|23|41.2}} | 6.46 | 1.46 | 326 | F2II | suspected variable |
| HD 54967 | 54967 | 34350 | 07|07|16.28}} | −59|42|59.2}} | 6.46 | −1.79 | 1455 | B3V |
| HD 93738 | 93738 | 52815 | 10|47|53.55}} | −64|15|46.3}} | 6.46 | 0.67 | 469 | B9.5V | in IC 2602 |
| HD 49219 | 49219 | 32269 | 06|44|12.81}} | −54|41|43.9}} | 6.47 | −0.30 | 736 | B5/B6V | 0.011|1.60}} |
| HD 70267 | 70267 | 40655 | 08|17|55.79}} | −59|10|00.3}} | 6.47 | 2.01 | 254 | F5V |
| V487 Car | V487 | 84809 | 47893 | 09|45|40.64}} | −57|11|09.8}} | 6.47 | −0.66 | 869 | B8III/IV | α2 CVn variable |
| HD 93695 | 93695 | 52806 | 10|47|44.34}} | −59|52|30.9}} | 6.47 | −1.41 | 1230 | B5Vvar |
| HD 95122 | 95122 | 53556 | 10|57|20.22}} | −69|02|17.0}} | 6.48 | −0.55 | 832 | B7V | suspected variable |
| HD 92399 | 92399 | 52103 | 10|38|45.39}} | −59|15|44.7}} | 6.50 | −1.82 | 1502 | B4/B5III/IV |
| HD 96248 | V414 | 96248 | 54179 | 11|04|57.57}} | −59|51|32.0}} | 6.58 | 3700 | B1Iab | α Cyg variable, {{Variable star|6.53|6.62|8.52}} |
| HD 57853 | 57853 | 35564 | 07|20|21.43}} | −52|18|31.91}} | 6.63 | 113 | F9V | component of the HIP 35564 system |
| QX Car | QX | 86118 | 48589 | 09|54|33.88}} | −58|25|16.6}} | 6.64 | 1610 | B2V | Algol variable, {{Variable star|6.6|7.21|4.48}} |
| HD 96446 | V430 | 96446 | 54266 | 11|06|05.82}} | −59|56|59.6}} | 6.68 | 1540 | B2k | β Cep variable, {{VSA|0.03}} |
| HD 53143 | 53143 | 33690 | 06|59|59.66}} | −61|20|10.3}} | 6.68 | 59.74 | G9V | has a circumstellar disk |
| VY Car | VY | 93203 | 52538 | 10|44|32.69}} | −57|33|55.3}} | 6.91 | 9100 | F7Iab/Ib | classical Cepheid, {{Variable star|6.91|8.00|18.89}} |
| AG Car | AG | 94910 | 53461 | 10|56|11.58}} | −60|27|12.8}} | 6.96 | 17000 | B2-3Ib/WN11 | luminous blue variable, {{Variable star|5.7|8.3|371.4}} |
| BO Car | BO | 93420 | 10|45|50.63}} | −59|29|19.5}} | 7.18 | M4Iab: | semiregular variable, {{Variable star|7.15|7.95|130.7}} |
| HD 93403 | 93403 | 52628 | 10|45|44.12}} | −59|24|28.1}} | 7.30 | 2670 | O5.5I+O7V | binary star |
| HD 93129A | 93129A | 10|43|57.46}} | −59|32|51.2}} | 7.31 | 7500 | O2If*+O3.5 | in Trumpler 14; binary star; primary is one of the most luminous stars known |
| V Car | V | 72275 | 41588 | 08|28|43.70}} | −60|07|21.3}} | 7.31 | 5600 | G2Iab: | classical Cepheid, {{Variable star|7.08|7.82|6.70}} |
| HD 93843 | 93843 | 10|48|37.78}} | −60|13|25.5}} | 7.33 | O5III(f)v | irregular variable, {{Variable star|7.31|7.35}} |
| HD 95086 | 95086 | 53524 | 10|57|03.0}} | -68|40|02}} | 7.36 | 295 | A8III | has a planet (b) |
| HD 93250 | 93250 | 52558 | 10|44|45.03}} | −59|33|54.7}} | 7.50 | 7500 | O4IIIfc | in Trumpler 16; suspected variable |
| HR Car | HR | 90177 | 50843 | 10|22|53.84}} | −59|37|28.4}} | 7.57 | 17700 | B3Iaep | luminous blue variable, {{Variable star|6.8|8.80}} |
| WR 40 | V385 | 96548 | 54283 | 11|06|17.20}} | −65|30|35.2}} | 7.70 | 5900 | WN8h | Wolf–Rayet star and rotating ellipsoidal variable, {{VSA|0.04|4.76}}; one of the most luminous stars known |
| HD 93205 | V560 | 93205 | 10|44|33.74}} | −59|44|15.5}} | 7.75 | 7500 | O3.5V((f+)) | in Trumpler 16; rotating ellipsoidal variable, {{Variable star|7.74|7.76|6.08}} |
| IW Car | IW | 82084
82085 | 09|26|53.30}} | −63|37|48.9}} | 7.90 | A4Iab/II: | RV Tau variable, {{Variable star|7.77|9.10|143.6}} |
| HD 65216 | 65216 | 38558 | 07|53|41.3}} | −63|38|50.4}} | 7.98 | 112 | G5V | has two planets (b & c) |
| HD 97152 | V431 | 97152 | 54574 | 11|10|04.08}} | −60|58|45.0}} | 8.07 | 4000 | WC7+O7V | Wolf–Rayet star; eclipsing binary, {{Variable star|7.97|8.08|1.62}} |
| HD 63765 | 63765 | 38041 | 07|47|49.72}} | −54|15|50.9}} | 8.10 | 5.53 | 106 | G9V | has a planet (b) |
| Y Car | Y | 91565 | 51653 | 10|33|10.85}} | −58|29|55.1}} | 8.16 | 3050 | F2 | double-mode Cepheid, {{Variable star|7.53|8.48|3.64}} |
| HD 51608 | 51608 | 33229 | 06|54|51}} | −55|15|34}} | 8.17 | 114 | K0IV | has two planets (b & c) |
| YZ Car | YZ | 90912 | 51262 | 10|28|16.85}} | −59|21|00.7}} | 8.24 | 5900 | G5 | classical Cepheid, {{Variable star|8.24|9.08|18.17}} |
| WR 16 | V396 | 86161 | 48617 | 09|54|52.90}} | −57|43|38.3}} | 8.32 | WN8h | rotating ellipsoidal variable, {{VSA|0.06}}; one of the most luminous stars known |
| EM Car | EM | 97484 | 11|12|04.51}} | −61|05|42.9}} | 8.52 | O8V | Algol variable |
| RT Car | RT | 303310 | 52562 | 10|44|47.15}} | −59|24|48.1}} | 8.55 | 1430 | M2Iab: | possibly in Trumpler 15; irregular variable, {{Variable star|8.2|9.9}}, one of the largest stars known |
| HD 85567 | V596 | 85567 | 48269 | 09|50|28.54}} | −60|58|03.0}} | 8.57 | 6900 | B2 | FS CMa variable, {{Variable star|8.44|8.75}} |
| UX Car | UX | 91039 | 51338 | 10|29|11.24}} | −57|36|48.3}} | 8.62 | 2530 | F2II | classical Cepheid, {{Variable star|7.81|8.67|3.68}} |
| XZ Car | XZ | 305996 | 54101 | 11|04|13.47}} | −60|58|47.7}} | 8.67 | B2:pe | classical Cepheid, {{Variable star|8.05|9.12|16.65}} |
| GG Car | GG | 94878 | 53444 | 10|55|58.92}} | −60|23|33.4}} | 8.70 | B0/2eq | Be star and re-radiating binary system, {{Variable star|8.44|9.08|31.03}} |
| V403 Car | V403 | 10|35|40.67}} | −58|12|44.6}} | 8.74 | 8400 | B1III | in NGC 3293; β Cep variable, {{VSA|0.033|0.25}} |
| Tr 16-104 | V572 | 10|44|47.31}} | −59|43|53.2}} | 8.75 | 7500 | O7V((f))+
O9.5V+
B0.2IV | in Trumpler 16; Algol variable, {{Variable star|8.66|9.07|2.15}} |
| V348 Car | V348 | 90707 | 10|29|59.00}} | −57|40|32.8}} | 8.78 | B1III | β Lyr variable, {{Variable star|8.55|8.93|5.56}} |
| WR 25 | V396 | 93162 | 10|44|10.34}} | −59|43|11.4}} | 8.80 | 7500 | O2.5If*/WN6 | in Trumpler 16; Wolf–Rayet star; one of the most luminous stars known |
| HD 60435 | V409 | 60435 | 36537 | 07|30|56.99}} | −57|59|28.2}} | 8.89 | 739 | Ap... | rapidly oscillating Ap star |
| WR 23 | 92809 | 52331 | 10|41|38.32}} | −58|46|18.7}} | 9.03 | 3400 | WC6 | Wolf–Rayet star |
| HD 92024 | V381 | 92024 | 10|36|08.31}} | −58|13|04.77}} | 9.04 | 8400 | B1III | in NGC 3293; β Cep variable, {{Variable star|9.04|9.06|0.17}} |
| GH Car | GH | 306077 | 54621 | 11|10|44.59}} | −60|45|01.0}} | 9.20 | G0 | classical Cepheid, {{Variable star|9|9.35|5.73}} |
| WZ Car | WZ | 94777 | 53397 | 10|55|18.73}} | −60|56|24.0}} | 9.37 | 4700 | F8 | classical Cepheid, {{Variable star|8.63|9.88|23.02}} |
| CPD -59° 2635 | V731 | 10|45|12.72}} | −59|44|46.2}} | 9.43 | 7500 | O8V+O9.5V | in Trumpler 16; Algol variable, {{Variable star|9.27|9.78|2.30}} |
| V392 Car | V392 | 07|58|10.47}} | −60|51|57.5}} | 9.49 | A2Vp... | in NGC 2516; Algol and α2 CVn variable, {{Variable star|9.49|9.67}} |
| XY Car | XY | 308149 | 53945 | 11|02|16.07}} | −64|15|46.5}} | 9.49 | G5 | classical Cepheid, {{Variable star|8.82|9.77|12.43}} |
| HD 87643 | V640 | 87643 | 10|04|30.29}} | −58|39|52.1}} | 9.50 | B2e | Orion variable, {{Variable star|7.4|9.8}} |
| CPD -59 2628 | V573 | 10|45|08.23}} | −59|40|49.5}} | 9.52 | 7500 | O9.5V+B0.3V | in Trumpler 16; Algol variable |
| HD 90657 | V398 | 90657 | 51109 | 10|26|31.41}} | −58|38|26.2}} | 9.69 | 3500 | WN5+O4-6 | Wolf–Rayet star; eclipsing binary, {{VSA|0.035}} |
| GL Car | GL | 306168 | 11|14|39.84}} | −60|39|36.3}} | 9.70 | B3:V | Algol variable |
| DW Car | DW | 305543 | 10|43|10.07}} | −60|02|11.7}} | 9.85 | B2:pe | in Collinder 228; Algol variable |
| SS73 17 | V648 | 10|11|02.95}} | −57|48|13.9}} | 9.99 | M3pe+OB | Z And variable, {{Variable star|9.6|10.0|520}} |
| CPD -57 2874 | 10|15|21.97}} | −57|51|42.7}} | 10.16 | sgB1[e] | B[e] star |
| GZ Car | GZ | 302719 | 50615 | 10|20|20.37}} | −59|22|35.8}} | 10.20 | 2400 | G5 | double-mode Cepheid, {{Variable star|9.98|10.47|4.16}} |
| HH Car | HH | 303503 | 10|53|36.47}} | −59|27|18.2}} | 10.31 | B | Algol variable, {{Variable star|10.3|10.82|3.23}} |
| EY Car | EY | 52380 | 10|42|23.03}} | −61|09|57.3}} | 10.35 | B2:pe | double-mode Cepheid, {{Variable star|10.01|10.56|2.88}} |
| HD 307938 | V557 | 307938 | 10|42|41.52}} | −64|21|04.4}} | 10.57 | G2V | BY Dra variable, {{VSA|0.21}} |
| WR 18 | V500 | 89358 | 50368 | 10|17|02.27}} | −57|54|47.9}} | 10.6 | 6300 | WN4-s | Wolf–Rayet star |
| HD 94546 | V428 | 94546 | 53274 | 10|53|44.82}} | −59|30|46.7}} | 10.7 | WN4+O8V | Wolf–Rayet star; eclipsing binary, {{VSA|0.05}} |
| He 3-519 | 10|53|59.59}} | −60|26|44.3}} | 10.85 | WN11 | Wolf–Rayet star, {{Variable star|10.6|11.0}} |
| NGC 3603-A1 | 97950A | 11|15|07.31}} | −61|15|38.4}} | 11.12 | 20000 | WN6ha+O3V | in NGC 3603; Algol variable, {{VSA|0.45|3.77}} both components among the most luminous and massive stars known |
| CR Car | CR | 10|32|54.07}} | −58|31|15.5}} | 11.30 | B2:pe | classical Cepheid, {{Variable star|11.3|11.89|9.76}} |
| NGC 3603-B | 97950B | 11|15|07.41}} | −61|15|38.6}} | 11.33 | WN6h+abs | one of the most luminous and most massive stars known |
| Innes' star | 11|16|00.21}} | −57|32|51.6}} | 11.52 | 41.31 | M3.5 | has a planet |
| QU Car | QU | 310376 | 54226 | 11|05|42.49}} | −68|37|58.2}} | 11.54 | 1290 | B+... | V Sge variable, {{Variable star|10.9|11.7|0.45}} |
| WR 30 | V541 | 94305 | 10|51|06.01}} | −62|17|01.7}} | 11.73 | WC6+O7.5V | Algol variable, {{VSA|0.09}} |
| WRA 751 | V432 | 11|08|40.06}} | −60|42|51.7}} | 11.79 | WR: | luminous blue variable, {{Variable star|10.7|12.43}} |
| NGC 3603-C | 97950C | 11|15|07.59}} | −61|15|18.0}} | 11.89 | WN6h+abs | spectroscopic binary |
| FO 15 | V662 | 10|45|36.32}} | −59|48|23.2}} | 12.09 | 7500 | O5.5V+O9.5V | in Trumpler 16; Algol variable, {{Variable star|12.09|12.7|1.41}} |
| Sher 25 | 11|15|07.8}} | −61|15|17}} | 12.27 | B1.5Iab | in NGC 3603; potential supernova progenitor |
| WR 30a | V574 | 10|51|38.93}} | −60|56|35.2}} | 12.73 | WR+... | Algol variable, {{VSA|0.05}} |
| He 2-38 | V366 | 09|54|43.29}} | −57|18|52.4}} | 12.92 | M5-7.5 | Mira and Z And variable, {{Variable star|12.1|14.4|433}} |
| BPM 6502 | V727 | 10|44|10.23}} | −69|18|18.0}} | 13.09 | DA2.2+M | re-radiating binary system |
| WR 20a | V712 | 10|23|58.00}} | −57|45|49.0}} | 13.5 | O3If*/WN6+
O3If*/WN6 | in Westerlund 2; Algol variable |
| LHS 288 | 10|44|21.32}} | −61|12|38.4}} | 13.92 | 15.602 | M4 | |
| OGLE-TR-113 | V752 | 10|52|24.4}} | −61|26|48.5}} | 14.42 | 1800 | K | has a transiting planet (b) |
| 2S 0921-630 | V395 | 09|22|35.20}} | −63|17|38.5}} | 15.3 | K0IIIe | low-mass X-ray binary |
| OGLE-TR-123 | V816 | 11|06|51.1}} | −61|11|10.5}} | 15.47 | FV+MV | possibly has a transiting planet |
| OGLE-TR-111 | V759 | 10|53|17.9}} | −61|24|20.3}} | 15.55 | 5000 | G | has a transiting planet (b) and
a possible second planet |
| OGLE-TR-132 | V742 | 10|50|34.7}} | −61|57|25.9}} | 15.72 | 7110 | F | has a transiting planet (b) |
| OY Car | OY | 10|06|22.07}} | −70|14|04.6}} | 16.2 | 277 | M5/M6:... | SU UMa variable and eclipsing binary, {{Variable star|11.2|16.2|0.063}} |
| OGLE-TR-182 | 11|09|18.73}} | −61|05|42.93}} | 16.84 | 12700 | G | has a transiting planet (b) |
| OGLE-TR-211 | 10|40|14.39}} | −62|27|20.2}} | 5300 | F | has a transiting planet (b) |
| OGLE-TR-122 | V817 | 11|06|52.0}} | −60|51|45.7}} | has a transiting brown dwarf |
| OGLE2-TR-L9 | 11|07|55}} | −61|08|46}} | 2935 | F3 | has a transiting planet (b) |
| 1E 1048.1-5937 | 10|50|08.93}} | −59|53|19.9}} | Be | anomalous X-ray pulsar |
| DENIS J081730.0-615520 | 08|17|30.01}} | −61|55|15.8}} | 16.1 | T6 | brown dwarf |
| PSR J1048-5832 | 10|48|12.20}} | −58|32|05.8}} | pulsar |
| PSR J1119-6127 | 11|19|14.30}} | −61|27|49.5}} | pulsar{{Starlist Legend}} |
1. ^{{cite book |author= Kunitzsch, P., & Smart, T., |date = 2006 |title = A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations |edition = 2nd rev. |publisher = Sky Pub |location = Cambridge, MA |isbn = 978-1-931559-44-7 |page = 25}}