# List of stars in Carina

This is the list of notable stars in the constellation Carina, sorted by decreasing brightness.
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$^h$ 23$^m$ 57.09$^s$ | −52° 41′ 44.6″ | −0.72 | −5.53 | 313 | A9 II | Suhel; 2nd brightest star |
| β Car | β | | 80007 | 45238 | 09$^h$ 13$^m$ 12.24$^s$ | −69° 43′ 02.9″ | 1.67 | −0.99 | 111 | A1 III | Miaplacidus |
| ε Car | ε | | 71129 | 41037 | 08$^h$ 22$^m$ 30.86$^s$ | −59° 30′ 34.3″ | 1.86 | −4.58 | 632 | K3III+B2V | Avior; suspected eclipsing binary, V$_{max}$ = 1.82$^m$, V$_{min}$ = 1.94$^m$ |
| ι Car | ι | | 80404 | 45556 | 09$^h$ 17$^m$ 05.43$^s$ | −59° 16′ 30.9″ | 2.23 | −4.43 | 692 | A8Ib | Aspidiske, Turais, Scutulum; suspected variable, V$_{max}$ = 2.23$^m$, V$_{min}$ = 2.28$^m$ |
| θ Car | θ | | 93030 | 52419 | 10$^h$ 42$^m$ 57.43$^s$ | −64° 23′ 40.1″ | 2.74 | −2.91 | 439 | B0Vp | in IC 2602 |
| υ Car | υ | | 85123 | 48002 | 09$^h$ 47$^m$ 06.14$^s$ | −65° 04′ 19.3″ | 2.92 | −5.56 | 1622 | A9 | binary star |
| ω Car | ω | | 89080 | 50099 | 10$^h$ 13$^m$ 44.28$^s$ | −70° 02′ 16.5″ | 3.29 | −1.99 | 370 | B8III | |
| p Car | p | PP | 91465 | 51576 | 10$^h$ 32$^m$ 01.48$^s$ | −61° 41′ 07.3″ | 3.30 | −2.62 | 497 | B4Vne | γ Cas variable, V$_{max}$ = 3.22$^m$, V$_{min}$ = 3.55$^m$ |
| V337 Car | q | V337 | 89388 | 50371 | 10$^h$ 17$^m$ 05.01$^s$ | −61° 19′ 56.4″ | 3.39 | −3.38 | 736 | K3II | irregular variable, V$_{max}$ = 3.36$^m$, V$_{min}$ = 3.44$^m$ |
| a Car | a | V357 | 79351 | 45080 | 09$^h$ 10$^m$ 58.11$^s$ | −58° 58′ 00.9″ | 3.43 | −2.11 | 418 | B2IV | eclipsing binary, V$_{max}$ = 3.41$^m$, V$_{min}$ = 3.44$^m$ |
| χ Car | χ | | 65575 | 38827 | 07$^h$ 56$^m$ 46.74$^s$ | −52° 58′ 56.6″ | 3.46 | −1.91 | 387 | B3IVp | β Cep variable, ΔV = 0.015$^m$, P = 0.10 d |
| l Car | l | | 84810 | 47854 | 09$^h$ 45$^m$ 14.83$^s$ | −62° 30′ 28.5″ | 3.69 | −4.64 | 1509 | G5Iab/Ib | classical Cepheid, V$_{max}$ = 3.28$^m$, V$_{min}$ = 4.18$^m$, P = 35.54 d |
| HD 94510 | u | | 94510 | 53253 | 10$^h$ 53$^m$ 29.57$^s$ | −58° 51′ 11.8″ | 3.78 | 1.42 | 97 | K0III-IV... | suspected variable, V$_{max}$ = 3.75$^m$, V$_{min}$ = 3.80$^m$ |
| HD 90853 | s | | 90853 | 51232 | 10$^h$ 27$^m$ 52.75$^s$ | −58° 44′ 21.9″ | 3.81 | −3.71 | 1042 | F2II | suspected variable |
| HD 76728 | c | | 76728 | 43783 | 08$^h$ 55$^m$ 02.86$^s$ | −60° 38′ 41.0″ | 3.84 | −1.06 | 312 | B8III | double star |
| V382 Car | x | V382 | 96918 | 54463 | 11$^h$ 08$^m$ 35.40$^s$ | −58° 58′ 30.2″ | 3.93 | −7.37 | 5927 | G0Ia0 | hypergiant; slow irregular variable, V$_{max}$ = 3.77$^m$, V$_{min}$ = 4.05$^m$ |
| HD 79447 | i | | 79447 | 45101 | 09$^h$ 11$^m$ 16.77$^s$ | −62° 19′ 01.3″ | 3.96 | −1.97 | 499 | B3IV | variable star, ΔV = 0.008$^m$, P = 22.26 d |
| HD 90589 | I | | 90589 | 50954 | 10$^h$ 24$^m$ 23.74$^s$ | −74° 01′ 53.6″ | 3.99 | 2.94 | 53 | F2IV | suspected variable, V$_{max}$ = 3.96$^m$, V$_{min}$ = 4.00$^m$ |
| HD 83183 | h | | 83183 | 46974 | 09$^h$ 34$^m$ 26.66$^s$ | −59° 13′ 47.2″ | 4.08 | −4.83 | 1976 | B5II | |
| V343 Car | d | V343 | 74375 | 42568 | 08$^h$ 40$^m$ 37.04$^s$ | −59° 45′ 39.7″ | 4.31 | −3.87 | 1411 | B1.5III | β Cep variable |
| HD 80230 | g | | 80230 | 45496 | 09$^h$ 16$^m$ 12.10$^s$ | −57° 32′ 29.2″ | 4.34 | −1.74 | 536 | M1III | suspected variable, V$_{max}$ = 4.31$^m$, V$_{min}$ = 4.35$^m$ |
| HD 47306 | N | | 47306 | 31407 | 06$^h$ 34$^m$ 58.59$^s$ | −52° 58′ 32.3″ | 4.35 | −4.31 | 1762 | B9III | |
| HR 2554 | A | V415 | 50337 | 32761 | 06$^h$ 49$^m$ 51.32$^s$ | −53° 37′ 21.0″ | 4.39 | −1.74 | 553 | G6II | Algol variable, ΔV = 0.06$^m$ |
| HD 91942 | r | | 91942 | 51849 | 10$^h$ 35$^m$ 35.31$^s$ | −57° 33′ 27.5″ | 4.45 | −3.68 | 1376 | K3/K4II | suspected variable |
| η Car | η | | 93308 | | 10$^h$ 45$^m$ 03.60$^s$ | −59° 41′ 03.0″ | 4.47 | | 7500 | LBV | Foramen, Tseen She; in Trumpler 16; binary star; luminous blue variable, V$_{max}$ = −0.8$^m$, V$_{min}$ = 7.9$^m$; surrounded by the Homunculus Nebula; one of the most luminous and most massive stars known. |
| HR 3643 | G | | 78791 | 44599 | 09$^h$ 05$^m$ 08.83$^s$ | −72° 36′ 09.7″ | 4.47 | −1.25 | 454 | F6II-III | |
| V344 Car | f | V344 | 75311 | 43105 | 08$^h$ 46$^m$ 42.56$^s$ | −56° 46′ 11.3″ | 4.50 | −1.62 | 546 | B3Vne | γ Cas variable, V$_{max}$ = 4.40$^m$, V$_{min}$ = 4.51$^m$ |
| HD 83944 | m | | 83944 | 47391 | 09$^h$ 39$^m$ 21.04$^s$ | −61° 19′ 41.2″ | 4.51 | 0.33 | 224 | B9V | suspected variable |
| V520 Car | w | V520 | 93070 | 52468 | 10$^h$ 43$^m$ 32.31$^s$ | −60° 33′ 59.9″ | 4.58 | −2.99 | 1065 | K3Ib | irregular variable, V$_{max}$ = 4.50$^m$, V$_{min}$ = 4.59$^m$ |
| V533 Car | y | V533 | 97534 | 54751 | 11$^h$ 12$^m$ 36.02$^s$ | −60° 19′ 03.5″ | 4.59 | −8.34 | 12538 | A6Ia | α Cyg variable |
| HD 96566 | z$^1$ | | 96566 | 54301 | 11$^h$ 06$^m$ 32.47$^s$ | −62° 25′ 26.9″ | 4.62 | −0.65 | 370 | G8III | |
| V399 Car | P | V399 | 90772 | 51192 | 10$^h$ 27$^m$ 24.48$^s$ | −57° 38′ 19.7″ | 4.65 | | | A6Ia | semiregular variable, V$_{max}$ = 4.63$^m$, V$_{min}$ = 4.72$^m$, P = 88.3 d |
| V345 Car | E | V345 | 78764 | 44626 | 09$^h$ 05$^m$ 38.38$^s$ | −70° 32′ 18.7″ | 4.67 | −2.94 | 1079 | B2IVe | γ Cas variable, V$_{max}$ = 4.67$^m$, V$_{min}$ = 4.78$^m$, P = 137.7 d |
| HD 92397 | t$^2$ | | 92397 | 52102 | 10$^h$ 38$^m$ 45.01$^s$ | −59° 10′ 58.8″ | 4.69 | −4.08 | 1852 | K4/K5III: | suspected variable |
| HD 91375 | K | | 91375 | 51438 | 10$^h$ 30$^m$ 20.08$^s$ | −71° 59′ 33.8″ | 4.72 | 0.22 | 259 | A2III | |
| HR 3220 | B | | 68456 | 39903 | 08$^h$ 09$^m$ 00.86$^s$ | −61° 18′ 06.1″ | 4.74 | 3.09 | 70 | F5V | |
| V518 Car | | V518 | 92938 | 52370 | 10$^h$ 42$^m$ 14.14$^s$ | −64° 27′ 59.2″ | 4.76 | −0.97 | 456 | B3V | in IC 2602; γ Cas variable |
| HD 81101 | k | | 81101 | 45856 | 09$^h$ 20$^m$ 56.83$^s$ | −62° 24′ 16.7″ | 4.79 | 0.62 | 223 | G6III | |
| HD 93194 | | | 93194 | 52502 | 10$^h$ 44$^m$ 06.94$^s$ | −63° 57′ 40.0″ | 4.80 | −1.06 | 484 | B5Vn | in IC 2602; suspected irregular variable, V$_{max}$ = 4.79$^m$, V$_{min}$ = 4.84$^m$ |
| HD 66591 | D | | 66591 | 39138 | 08$^h$ 00$^m$ 19.97$^s$ | −63° 34′ 03.0″ | 4.81 | −1.29 | 542 | B3V | suspected variable |
| HD 73389 | e$^2$ | | 73389 | 42134 | 08$^h$ 35$^m$ 19.65$^s$ | −58° 00′ 33.5″ | 4.84 | 0.60 | 229 | K0III | |
| HD 93607 | | | 93607 | 52736 | 10$^h$ 46$^m$ 51.24$^s$ | −64° 23′ 00.6″ | 4.87 | −0.83 | 449 | B3IV | in IC 2602; suspected variable |
| HD 61248 | Q | | 61248 | 36942 | 07$^h$ 35$^m$ 39.70$^s$ | −52° 32′ 01.7″ | 4.93 | −0.48 | 394 | K3III | suspected variable |
| V376 Car | b$^1$ | V376 | 77002 | 43937 | 08$^h$ 56$^m$ 58.43$^s$ | −59° 13′ 45.7″ | 4.93 | −1.47 | 621 | B2IV-V | β Cep variable, V$_{max}$ = 4.91$^m$, V$_{min}$ = 4.96$^m$, P = 0.021 d |
| HD 91496 | | | 91496 | 51495 | 10$^h$ 31$^m$ 02.07$^s$ | −73° 13′ 17.4″ | 4.94 | −2.42 | 964 | K4/K5III | suspected variable, V$_{max}$ = 4.87$^m$, V$_{min}$ = 4.97$^m$ |
| HD 90264 | L | | 90264 | 50847 | 10$^h$ 22$^m$ 58.18$^s$ | −66° 54′ 05.5″ | 4.97 | −0.63 | 430 | B8V | |
| HD 92063 | t$^1$ | | 92063 | 51912 | 10$^h$ 36$^m$ 20.56$^s$ | −59° 33′ 51.5″ | 5.08 | 0.50 | 269 | K1III | |
| HD 59219 | | | 59219 | 36114 | 07$^h$ 26$^m$ 21.86$^s$ | −51° 01′ 06.6″ | 5.09 | −1.09 | 562 | K0III | |
| HD 96919 | z$^2$ | V371 | 96919 | 54461 | 11$^h$ 08$^m$ 34.01$^s$ | −61° 56′ 49.8″ | 5.12 | −6.03 | 5525 | B9Ia | α Cyg variable, V$_{max}$ = 5.12$^m$, V$_{min}$ = 5.19$^m$ |
| HD 53047 | | | 53047 | 33779 | 07$^h$ 00$^m$ 51.51$^s$ | −51° 24′ 09.5″ | 5.14 | −1.25 | 617 | M1III | semiregular variable |
| V386 Car | | V386 | 54118 | 34105 | 07$^h$ 04$^m$ 18.32$^s$ | −56° 44′ 59.0″ | 5.14 | 0.45 | 282 | A0p: | α$^2$ CVn variable, ΔV = 0.026$^m$, P = 3.28 d |
| HD 88981 | M | | 88981 | 50083 | 10$^h$ 13$^m$ 30.68$^s$ | −66° 22′ 22.2″ | 5.15 | 0.31 | 304 | Am | |
| HD 69863 | C | | 69863 | 40429 | 08$^h$ 15$^m$ 15.95$^s$ | −62° 54′ 56.2″ | 5.16 | 0.81 | 242 | A+... | binary star |
| HD 77370 | b$^2$ | | 77370 | 44143 | 08$^h$ 59$^m$ 24.38$^s$ | −59° 05′ 03.8″ | 5.17 | 3.08 | 85 | F3V | |
| HR 3153 | | V460 | 66342 | 39070 | 07$^h$ 59$^m$ 37.55$^s$ | −60° 35′ 13.5″ | 5.19 | −2.34 | 1045 | M0II | in NGC 2516; semiregular variable, V$_{max}$ = 5.15$^m$, V$_{min}$ = 5.3$^m$ |
| HD 97583 | | | 97583 | 54767 | 11$^h$ 12$^m$ 45.27$^s$ | −64° 10′ 11.2″ | 5.22 | 0.30 | 314 | B9V | double star |
| HD 93549 | | | 93549 | 52701 | 10$^h$ 46$^m$ 29.61$^s$ | −64° 15′ 47.7″ | 5.23 | −0.37 | 429 | B7IV | in IC 2602 |
| HD 88323 | | | 88323 | 49698 | 10$^h$ 08$^m$ 42.84$^s$ | −65° 48′ 55.9″ | 5.26 | 0.16 | 341 | K0III | optical double |
| V524 Car | | V524 | 94367 | 53154 | 10$^h$ 52$^m$ 30.85$^s$ | −57° 14′ 25.5″ | 5.26 | −6.08 | 6037 | B9Ia | α Cyg variable |
| HD 73390 | e$^1$ | | 73390 | 42129 | 08$^h$ 35$^m$ 15.58$^s$ | −58° 13′ 29.1″ | 5.27 | −2.08 | 962 | B3V+... | |
| HD 91056 | | | 91056 | 51313 | 10$^h$ 28$^m$ 52.60$^s$ | −64° 10′ 20.2″ | 5.27 | −4.64 | 3135 | K3Ib | slow irregular variable |
| HD 80951 | | | 80951 | 45581 | 09$^h$ 17$^m$ 25.21$^s$ | −74° 53′ 39.8″ | 5.28 | −1.44 | 721 | A1V | |
| HD 84121 | | | 84121 | 47479 | 09$^h$ 40$^m$ 42.60$^s$ | −57° 59′ 00.9″ | 5.30 | 1.16 | 220 | A3IV | |
| HD 93540 | | | 93540 | 52678 | 10$^h$ 46$^m$ 16.58$^s$ | −64° 30′ 52.5″ | 5.33 | −0.45 | 466 | B7:V | in IC 2602; suspected variable |
| HD 92964 | | V519 | 92964 | 52405 | 10$^h$ 42$^m$ 40.57$^s$ | −59° 12′ 56.8″ | 5.36 | −6.23 | 6792 | B2.5Ia | α Cyg variable, V$_{max}$ = 5.32$^m$, V$_{min}$ = 5.43$^m$, P = 14.68 d |
| HD 57917 | | | 57917 | 35589 | 07$^h$ 20$^m$ 38.81$^s$ | −52° 05′ 09.3″ | 5.38 | −0.52 | 493 | B9V | |
| HD 80671 | | | 80671 | 45571 | 09$^h$ 17$^m$ 17.40$^s$ | −68° 41′ 22.5″ | 5.38 | 2.75 | 109 | F4V | |
| HD 49689 | | | 49689 | 32494 | 06$^h$ 46$^m$ 52.69$^s$ | −51° 15′ 55.6″ | 5.39 | −1.83 | 906 | K1II/IIIp+G: | suspected variable |
| HD 73887 | | | 73887 | 42286 | 08$^h$ 37$^m$ 18.85$^s$ | −62° 51′ 12.3″ | 5.45 | 0.39 | 335 | K0III | |
| HD 82350 | | | 82350 | 46358 | 09$^h$ 27$^m$ 06.50$^s$ | −71° 36′ 07.5″ | 5.46 | 1.51 | 201 | K2III | |
| HD 83095 | H | | 83095 | 46741 | 09$^h$ 31$^m$ 36.32$^s$ | −73° 04′ 51.3″ | 5.46 | −1.47 | 791 | K4III | |
| HD 92207 | | V370 | 92207 | 52004 | 10$^h$ 37$^m$ 27.08$^s$ | −58° 44′ 00.0″ | 5.47 | −6.52 | 8150 | A0Ia | α Cyg variable, V$_{max}$ = 5.45$^m$, V$_{min}$ = 5.52$^m$, P = 1.33 d |
| V450 Car | | V450 | 53921 | 34000 | 07$^h$ 03$^m$ 15.11$^s$ | −59° 10′ 41.3″ | 5.50 | −0.35 | 482 | B9IV | 53 Per variable, ΔV = 0.02$^m$ |
| HD 92664 | | V364 | 92664 | 52221 | 10$^h$ 40$^m$ 11.46$^s$ | −65° 06′ 00.9″ | 5.51 | −0.26 | 466 | B9p Si | α$^2$ CVn variable, V$_{max}$ = 5.48$^m$, V$_{min}$ = 5.52$^m$, P = 1.67 d |
| HD 67364 | | | 67364 | 39566 | 08$^h$ 05$^m$ 03.71$^s$ | −53° 06′ 28.5″ | 5.52 | 0.11 | 393 | K3/K4III | |
| HD 79698 | | | 79698 | 45219 | 09$^h$ 12$^m$ 55.62$^s$ | −59° 24′ 50.3″ | 5.54 | −0.28 | 475 | G6II | |
| HD 85656 | | | 85656 | 48310 | 09$^h$ 50$^m$ 55.60$^s$ | −62° 44′ 42.5″ | 5.56 | −1.78 | 959 | K1IIICN... | |
| HD 64067 | | | 64067 | 38152 | 07$^h$ 49$^m$ 06.72$^s$ | −56° 24′ 37.4″ | 5.57 | −1.72 | 934 | G5II | |
| HD 46569 | | | 46569 | 31079 | 06$^h$ 31$^m$ 18.22$^s$ | −51° 49′ 34.3″ | 5.58 | 2.73 | 121 | F8V | |
| HD 96706 | | | 96706 | 54327 | 11$^h$ 06$^m$ 49.93$^s$ | −70° 52′ 40.6″ | 5.58 | −2.12 | 1128 | B2V | variable star, ΔV = 0.004$^m$, P = 1.74 d |
| HD 65907 | | | 65907 | 38908 | 07$^h$ 57$^m$ 46.30$^s$ | −60° 18′ 12.1″ | 5.59 | 4.54 | 53 | G2V... | |
| HD 76113 | | | 76113 | 43499 | 08$^h$ 51$^m$ 36.53$^s$ | −57° 38′ 01.0″ | 5.59 | −1.12 | 716 | B8III | |
| V448 Car | O | V448 | 49877 | 32531 | 06$^h$ 47$^m$ 18.71$^s$ | −55° 32′ 24.2″ | 5.60 | −0.72 | 598 | K5III | semiregular variable |
| HD 65273 | | | 65273 | 38656 | 07$^h$ 54$^m$ 53.39$^s$ | −57° 18′ 10.4″ | 5.62 | 0.51 | 343 | K3/K4III | |
| HD 68434 | | | 68434 | 39957 | 08$^h$ 09$^m$ 33.63$^s$ | −56° 05′ 07.7″ | 5.66 | 0.33 | 380 | A3m... | |
| HD 89715 | | | 89715 | 50520 | 10$^h$ 19$^m$ 05.12$^s$ | −64° 40′ 34.6″ | 5.66 | 0.90 | 292 | A1V | |
| V372 Car | | V372 | 64722 | 38438 | 07$^h$ 52$^m$ 29.75$^s$ | −54° 22′ 01.9″ | 5.69 | −2.56 | 1462 | B1.5IV | β Cep variable, ΔV = 0.027$^m$, P = 0.12 d |
| HD 88661 | | QY | 88661 | 49934 | 10$^h$ 11$^m$ 46.47$^s$ | −58° 03′ 38.0″ | 5.70 | −2.29 | 1294 | B2IVnpe | γ Cas variable, V$_{max}$ = 5.63$^m$, V$_{min}$ = 5.83$^m$ |
| S Car | | S | 88366 | 49751 | 10$^h$ 09$^m$ 22.01$^s$ | −61° 32′ 57.1″ | 5.71 | | 1780 | K5-M6e | Mira variable, V$_{max}$ = 4.5$^m$, V$_{min}$ = 9.9$^m$, P = 149.49 d |
| HD 97670 | | | 97670 | 54829 | 11$^h$ 13$^m$ 30.79$^s$ | −59° 37′ 09.5″ | 5.73 | −3.00 | 1821 | B1.5V | suspected variable |
| HD 65662 | | | 65662 | 38783 | 07$^h$ 56$^m$ 18.65$^s$ | −60° 31′ 35.3″ | 5.74 | −2.17 | 1244 | K4II | in NGC 2516 |
| HD 93163 | | | 93163 | 52487 | 10$^h$ 43$^m$ 51.21$^s$ | −64° 14′ 56.6″ | 5.75 | −1.71 | 1009 | B3:V | suspected eclipsing binary, ΔV = 0.03$^m$ |
| HD 66194 | | V374 | 66194 | 38994 | 07$^h$ 58$^m$ 50.56$^s$ | −60° 49′ 28.2″ | 5.77 | −1.72 | 1028 | B2IVnpe | in NGC 2516; γ Cas variable, V$_{max}$ = 5.72$^m$, V$_{min}$ = 5.84$^m$ |
| HD 81830 | | | 81830 | 46225 | 09$^h$ 25$^m$ 27.38$^s$ | −61° 57′ 02.2″ | 5.77 | 1.47 | 236 | A4V+... | |
| HD 64185 | | | 64185 | 38160 | 07$^h$ 49$^m$ 12.95$^s$ | −60° 17′ 02.5″ | 5.78 | 3.06 | 114 | F1V | spectroscopic binary |
| HD 76538 | | | 76538 | 43669 | 08$^h$ 53$^m$ 48.67$^s$ | −60° 21′ 14.2″ | 5.78 | −2.35 | 1376 | B5III | |
| HD 85655 | | | 85655 | 48339 | 09$^h$ 51$^m$ 12.03$^s$ | −59° 25′ 32.4″ | 5.79 | −1.01 | 746 | K2IIICNp... | |
| HD 77615 | | | 77615 | 44256 | 09$^h$ 00$^m$ 45.75$^s$ | −60° 57′ 49.8″ | 5.80 | −2.13 | 1259 | G8II | |
| HD 84152 | | | 84152 | 47498 | 09$^h$ 41$^m$ 02.10$^s$ | −57° 15′ 34.0″ | 5.80 | 0.57 | 362 | K0/K1III | |
| HD 88473 | | | 88473 | 49764 | 10$^h$ 09$^m$ 30.20$^s$ | −68° 40′ 58.2″ | 5.80 | −0.46 | 583 | A0IV | |
| HD 49517 | | | 49517 | 32402 | 06$^h$ 45$^m$ 53.72$^s$ | −52° 24′ 35.0″ | 5.81 | −2.32 | 1376 | K3III | |
| HD 93943 | | | 93943 | 52922 | 10$^h$ 49$^m$ 24.46$^s$ | −59° 19′ 25.6″ | 5.85 | −1.24 | 853 | B9.5IV/V | |
| HD 80950 | | | 80950 | 45585 | 09$^h$ 17$^m$ 27.63$^s$ | −74° 44′ 04.8″ | 5.86 | 1.32 | 264 | A0V | |
| HD 60060 | | | 60060 | 36444 | 07$^h$ 29$^m$ 59.74$^s$ | −52° 39′ 04.6″ | 5.87 | 0.84 | 330 | K0III | |
| HD 66441 | | | 66441 | 39184 | 08$^h$ 00$^m$ 49.96$^s$ | −54° 09′ 04.7″ | 5.87 | −0.79 | 700 | B5Vn | suspected variable |
| V482 Car | | V482 | 82536 | 46620 | 09$^h$ 30$^m$ 23.45$^s$ | −58° 21′ 42.9″ | 5.88 | −1.68 | 1058 | M2III | semiregular variable |
| V514 Car | | V514 | 92287 | 52043 | 10$^h$ 38$^m$ 02.66$^s$ | −57° 15′ 22.7″ | 5.89 | −2.08 | 1278 | B3IV | rotating ellipsoidal variable, V$_{max}$ = 5.88$^m$, V$_{min}$ = 5.92$^m$, P = 2.90 d |
| HD 82406 | | | 82406 | 46460 | 09$^h$ 28$^m$ 30.60$^s$ | −66° 42′ 07.2″ | 5.90 | 1.33 | 268 | A0V | |
| HD 82347 | | | 82347 | 46482 | 09$^h$ 28$^m$ 47.19$^s$ | −62° 16′ 23.5″ | 5.91 | 0.06 | 482 | K1III | |
| HD 87283 | | | 87283 | 49164 | 10$^h$ 02$^m$ 00.11$^s$ | −60° 25′ 15.2″ | 5.93 | −4.03 | 3196 | A9IV | possibly in NGC 3114 |
| HD 90454 | | | 90454 | 50993 | 10$^h$ 24$^m$ 59.50$^s$ | −58° 34′ 34.7″ | 5.93 | 1.13 | 297 | F2III | |
| T Car | | T | 94776 | 53394 | 10$^h$ 55$^m$ 17.26$^s$ | −60° 31′ 01.9″ | 5.93 | 1.07 | 306 | K0III | not variable |
| HD 60228 | | | 60228 | 36496 | 07$^h$ 30$^m$ 30.91$^s$ | −54° 23′ 58.0″ | 5.95 | 0.33 | 433 | M1III | |
| HD 94683 | | | 94683 | 53334 | 10$^h$ 54$^m$ 29.60$^s$ | −61° 49′ 35.8″ | 5.95 | −2.59 | 1663 | K4III | suspected variable |
| HD 54732 | | | 54732 | 34349 | 07$^h$ 07$^m$ 13.30$^s$ | −51° 58′ 06.2″ | 5.96 | −0.23 | 564 | K0III | |
| HD 56705 | | | 56705 | 35084 | 07$^h$ 15$^m$ 21.27$^s$ | −52° 29′ 58.3″ | 5.96 | 0.58 | 389 | K0V | |
| HD 70839 | | | 70839 | 40932 | 08$^h$ 21$^m$ 12.10$^s$ | −57° 58′ 23.6″ | 5.96 | −3.36 | 2380 | B1.5III | |
| HD 92436 | | | 92436 | 52127 | 10$^h$ 38$^m$ 59.70$^s$ | −58° 49′ 00.8″ | 5.96 | −0.53 | 648 | M1III | |
| HD 91533 | | | 91533 | 51623 | 10$^h$ 32$^m$ 47.82$^s$ | −58° 40′ 00.3″ | 5.98 | −6.71 | 11241 | A2Iab | suspected variable |
| V522 Car | | V522 | 93737 | 52827 | 10$^h$ 48$^m$ 05.42$^s$ | −59° 55′ 09.0″ | 5.98 | | | A0Ia | α Cyg variable |
| HD 81613 | | | 81613 | 46101 | 09$^h$ 24$^m$ 05.50$^s$ | −61° 38′ 55.6″ | 5.99 | 0.92 | 337 | K0III | |
| HD 94650 | | | 94650 | 53272 | 10$^h$ 53$^m$ 42.13$^s$ | −70° 43′ 13.2″ | 5.99 | −0.89 | 776 | B6V | |
| HD 98560 | | | 98560 | 55280 | 11$^h$ 19$^m$ 16.84$^s$ | −64° 34′ 57.4″ | 5.99 | 3.12 | 122 | F6IV | |
| HD 90874 | | | 90874 | 51194 | 10$^h$ 27$^m$ 25.40$^s$ | −65° 42′ 17.0″ | 6.00 | 1.76 | 229 | A2V | |
| HD 53349 | | | 53349 | 33800 | 07$^h$ 01$^m$ 05.18$^s$ | −58° 56′ 25.1″ | 6.01 | 2.36 | 175 | F0V | suspected variable |
| HD 76346 | | | 76346 | 43620 | 08$^h$ 53$^m$ 03.80$^s$ | −56° 38′ 58.5″ | 6.02 | 1.23 | 296 | A0V | has a planet (b) |
| HD 80094 | | | 80094 | 45418 | 09$^h$ 15$^m$ 17.66$^s$ | −58° 23′ 18.2″ | 6.02 | 0.00 | 522 | B7IV | variable star, ΔV = 0.008$^m$, P = 1.56 d |
| HD 56239 | | | 56239 | 34780 | 07$^h$ 12$^m$ 01.98$^s$ | −63° 11′ 24.2″ | 6.03 | −0.29 | 598 | A0IV/V | |
| HD 57852 | | | 57852 | 35564 | 07$^h$ 20$^m$ 21.46$^s$ | −52° 18′ 42.8″ | 6.05 | | 113 | F5V | component of the HIP 35564 system; suspected variable |
| HD 82068 | | | 82068 | 46328 | 09$^h$ 26$^m$ 44.18$^s$ | −64° 55′ 47.5″ | 6.05 | 1.88 | 223 | A3Vn | |
| V390 Car | | V390 | 61966 | 37248 | 07$^h$ 39$^m$ 00.34$^s$ | −53° 16′ 24.2″ | 6.06 | −0.05 | 544 | B9IV-Vp... | α$^2$ CVn variable, ΔV = 0.004$^m$ |
| V535 Car | | V535 | 98292 | 55140 | 11$^h$ 17$^m$ 19.02$^s$ | −67° 49′ 24.6″ | 6.06 | −2.52 | 1698 | M2III | slow irregular variable |
| HD 88825 | | | 88825 | 50044 | 10$^h$ 13$^m$ 01.16$^s$ | −59° 55′ 05.1″ | 6.07 | −2.84 | 1976 | B4Ve | |
| HD 96544 | | | 96544 | 54294 | 11$^h$ 06$^m$ 29.30$^s$ | −58° 40′ 30.1″ | 6.07 | −1.81 | 1226 | K2II/III | |
| HD 92682 | | | 92682 | 52150 | 10$^h$ 39$^m$ 15.94$^s$ | −74° 29′ 36.2″ | 6.08 | −1.57 | 1105 | K3II | variable star, ΔV = 0.005$^m$, P = 0.084 d |
| HD 63382 | | | 63382 | 37854 | 07$^h$ 45$^m$ 35.52$^s$ | −56° 43′ 21.3″ | 6.10 | −1.20 | 942 | F0II | |
| R Car | | R | 82901 | 46806 | 09$^h$ 32$^m$ 14.60$^s$ | −62° 47′ 20.0″ | 6.10 | | 416 | M6.5 IIIpev | Mira variable, V$_{max}$ = 3.9$^m$, V$_{min}$ = 10.5$^m$, P = 308.71 d |
| HD 91619 | | V369 | 91619 | 51676 | 10$^h$ 33$^m$ 25.40$^s$ | −58° 11′ 24.6″ | 6.11 | −6.99 | 13583 | B7Ia | α Cyg variable, ΔV = 0.1$^m$, P = 1.12 d |
| U Car | | U | 95109 | 53589 | 10$^h$ 57$^m$ 48.19$^s$ | −59° 43′ 55.9″ | 6.11 | | | G3Ia | classical Cepheid, V$_{max}$ = 5.74$^m$, V$_{min}$ = 6.96$^m$, P = 38.83 d |
| HD 70982 | | | 70982 | 40926 | 08$^h$ 21$^m$ 07.65$^s$ | −64° 06′ 21.4″ | 6.11 | 0.34 | 464 | G6/G8III | |
| V461 Car | | V461 | 66546 | 39225 | 08$^h$ 01$^m$ 23.05$^s$ | −54° 30′ 56.0″ | 6.12 | −1.92 | 1320 | B2IV-V | Algol variable |
| HD 65908 | | | 65908 | 38863 | 07$^h$ 57$^m$ 12.76$^s$ | −63° 17′ 48.8″ | 6.14 | 0.37 | 464 | B8V | |
| V478 Car | | V478 | 80710 | 45615 | 09$^h$ 17$^m$ 51.67$^s$ | −67° 03′ 03.2″ | 6.14 | −1.96 | 1358 | K2III | semiregular variable |
| HD 87543 | | | 87543 | 49281 | 10$^h$ 03$^m$ 34.14$^s$ | −61° 53′ 02.6″ | 6.14 | −2.49 | 1734 | B4:Vne | |
| HD 95208 | | | 95208 | 53546 | 10$^h$ 57$^m$ 15.81$^s$ | −75° 05′ 59.2″ | 6.16 | −3.12 | 2345 | K1II | |
| HD 95324 | | | 95324 | 53701 | 10$^h$ 59$^m$ 14.05$^s$ | −61° 19′ 14.7″ | 6.16 | 0.93 | 363 | B8IV | |
| HD 96088 | | | 96088 | 54082 | 11$^h$ 04$^m$ 00.25$^s$ | −57° 57′ 19.2″ | 6.16 | −3.63 | 2964 | B3III | |
| HD 47001 | | | 47001 | 31265 | 06$^h$ 33$^m$ 26.31$^s$ | −52° 19′ 45.5″ | 6.18 | −0.17 | 607 | G8III | |
| V492 Car | | V492 | 86659 | 48782 | 09$^h$ 56$^m$ 59.84$^s$ | −69° 06′ 06.6″ | 6.18 | −1.43 | 1087 | B3V | 53 Per variable |
| HD 87436 | | | 87436 | 49233 | 10$^h$ 02$^m$ 59.95$^s$ | −60° 10′ 43.3″ | 6.18 | −3.80 | 3228 | A6II/III | suspected variable |
| HD 90630 | | | 90630 | 50976 | 10$^h$ 24$^m$ 44.56$^s$ | −73° 58′ 18.3″ | 6.18 | 0.53 | 441 | A2/A3V | suspected variable |
| V655 Car | | V655 | 91272 | 51425 | 10$^h$ 30$^m$ 08.81$^s$ | −66° 59′ 04.8″ | 6.19 | −1.70 | 1235 | B4IV | Algol variable, V$_{max}$ = 6.19$^m$, V$_{min}$ = 6.36$^m$, P = 16.93 d |
| HD 62897 | | | 62897 | 37599 | 07$^h$ 42$^m$ 53.36$^s$ | −58° 13′ 48.5″ | 6.20 | −0.23 | 629 | K0III | |
| HD 75086 | | | 75086 | 42936 | 08$^h$ 45$^m$ 05.55$^s$ | −58° 43′ 27.6″ | 6.20 | −1.23 | 997 | B7III | |
| HD 87238 | | | 87238 | 49160 | 10$^h$ 01$^m$ 58.09$^s$ | −57° 20′ 59.4″ | 6.20 | −0.62 | 753 | K1II | |
| HD 84850 | | | 84850 | 47913 | 09$^h$ 45$^m$ 55.82$^s$ | −58° 47′ 38.4″ | 6.22 | 1.68 | 264 | F5IV | |
| HD 89263 | | | 89263 | 50287 | 10$^h$ 16$^m$ 03.26$^s$ | −59° 54′ 12.4″ | 6.22 | 1.63 | 270 | A5V | |
| V532 Car | | V532 | 97451 | 54708 | 11$^h$ 12$^m$ 03.60$^s$ | −58° 25′ 24.1″ | 6.24 | −0.53 | 736 | M4III | semiregular variable |
| HD 91767 | | | 91767 | 51732 | 10$^h$ 34$^m$ 12.72$^s$ | −60° 59′ 15.5″ | 6.25 | −0.78 | 830 | K2/K3III | suspected variable |
| HD 65750 | | V341 | 65750 | 38834 | 07$^h$ 56$^m$ 50.70$^s$ | −59° 07′ 35.0″ | 6.25 | | 967 | M0III | semiregular variable, V$_{max}$ = 6.2$^m$, V$_{min}$ = 7.1$^m$ |
| HD 93344 | | | 93344 | 52520 | 10$^h$ 44$^m$ 20.10$^s$ | −70° 51′ 35.0″ | 6.25 | 1.12 | 346 | A5IV/V | |
| HD 52603 | | | 52603 | 33588 | 06$^h$ 58$^m$ 39.81$^s$ | −55° 43′ 44.1″ | 6.26 | 1.59 | 280 | K2III | |
| HD 74622 | | | 74622 | 42717 | 08$^h$ 42$^m$ 20.90$^s$ | −55° 46′ 28.8″ | 6.26 | 1.23 | 331 | K2III | |
| υ Car B | υ | | 85124 | | 09$^h$ 47$^m$ 06.70$^s$ | −65° 04′ 21.0″ | 6.26 | | 1623 | A8 Ib | component of the υ Car system |
| HD 93372 | | | 93372 | 52535 | 10$^h$ 44$^m$ 27.25$^s$ | −72° 26′ 37.1″ | 6.26 | 3.74 | 104 | F6V | |
| HD 93502 | | | 93502 | 52679 | 10$^h$ 46$^m$ 17.12$^s$ | −60° 36′ 10.4″ | 6.26 | 1.01 | 365 | A0IV | |
| HD 94491 | | | 94491 | 53231 | 10$^h$ 53$^m$ 21.18$^s$ | −58° 53′ 36.5″ | 6.26 | −2.16 | 1575 | B5V | |
| HD 82858 | | | 82858 | 46737 | 09$^h$ 31$^m$ 33.05$^s$ | −66° 43′ 08.6″ | 6.27 | −0.40 | 703 | K1III | |
| HD 66607 | | | 66607 | 39238 | 08$^h$ 01$^m$ 31.58$^s$ | −55° 27′ 16.8″ | 6.28 | −0.28 | 668 | B4V | |
| V375 Car | | V375 | 67536 | 39530 | 08$^h$ 04$^m$ 42.94$^s$ | −62° 50′ 10.9″ | 6.29 | | 1249 | B2.5Vn | β Cep variable, ΔV = 0.04$^m$, P = 1.02 d |
| HD 61031 | | | 61031 | 36856 | 07$^h$ 34$^m$ 39.58$^s$ | −51° 28′ 28.3″ | 6.29 | −1.76 | 1331 | A1III/IV | |
| HD 93662 | | | 93662 | 52797 | 10$^h$ 47$^m$ 38.41$^s$ | −57° 28′ 02.7″ | 6.29 | −3.35 | 2763 | M1II | suspected variable, V$_{max}$ = 6.28$^m$, V$_{min}$ = 6.41$^m$ |
| HD 94275 | | | 94275 | 53100 | 10$^h$ 51$^m$ 46.93$^s$ | −57° 16′ 20.3″ | 6.29 | −0.05 | 604 | A6III | |
| HD 63926 | | | 63926 | 38087 | 07$^h$ 48$^m$ 19.51$^s$ | −56° 28′ 15.9″ | 6.30 | −2.91 | 2264 | K0III+... | |
| HD 66341 | | | 66341 | 39073 | 07$^h$ 59$^m$ 40.09$^s$ | −60° 12′ 26.6″ | 6.30 | −1.81 | 1364 | B8III | in NGC 2516 |
| HD 81502 | | | 81502 | 46049 | 09$^h$ 23$^m$ 27.33$^s$ | −60° 18′ 08.4″ | 6.30 | −2.91 | 2264 | K1/K2II/III | |
| HD 86606 | | | 86606 | 48715 | 09$^h$ 56$^m$ 09.76$^s$ | −71° 23′ 21.5″ | 6.30 | −2.69 | 2050 | B1Ib | |
| HD 68423 | | | 68423 | 39843 | 08$^h$ 08$^m$ 24.65$^s$ | −63° 48′ 03.0″ | 6.32 | −0.58 | 782 | B6V | suspected variable |
| HD 80126 | | | 80126 | 45437 | 09$^h$ 15$^m$ 34.73$^s$ | −57° 34′ 39.9″ | 6.32 | −1.32 | 1098 | G8II | |
| QZ Car | | QZ | 93206 | 52526 | 10$^h$ 44$^m$ 22.92$^s$ | −59° 59′ 36.0″ | 6.32 | −3.23 | 2650 | B0Ib: | in Collinder 228; β Lyr variable, V$_{max}$ = 6.16$^m$, V$_{min}$ = 6.49$^m$, P = 6.00 d |
| HD 82458 | | | 82458 | 46407 | 09$^h$ 27$^m$ 49.19$^s$ | −71° 46′ 52.3″ | 6.33 | 2.57 | 184 | F3/F5V | |
| V486 Car | | V486 | 84416 | 47591 | 09$^h$ 42$^m$ 12.99$^s$ | −66° 54′ 53.4″ | 6.33 | 0.04 | 592 | A0V | β Lyr variable |
| HD 92536 | | | 92536 | 52160 | 10$^h$ 39$^m$ 22.85$^s$ | −64° 06′ 42.5″ | 6.33 | 0.49 | 479 | B8V | in IC 2602 |
| HD 74341 | | | 74341 | 42579 | 08$^h$ 40$^m$ 43.55$^s$ | −57° 32′ 43.9″ | 6.34 | 2.13 | 227 | A3V | |
| HD 90074 | | | 90074 | 50785 | 10$^h$ 22$^m$ 10.48$^s$ | −58° 15′ 56.3″ | 6.34 | 1.23 | 343 | G6III | |
| HD 90289 | | | 90289 | 50916 | 10$^h$ 23$^m$ 50.66$^s$ | −57° 57′ 14.1″ | 6.34 | −0.59 | 793 | K5Ib-II | suspected variable, V$_{max}$ = 6.33$^m$, V$_{min}$ = 6.35$^m$ |
| HD 93649 | | | 93649 | 52730 | 10$^h$ 46$^m$ 48.09$^s$ | −69° 12′ 35.3″ | 6.34 | −2.04 | 1545 | A2IV | |
| HD 97472 | | | 97472 | 54673 | 11$^h$ 11$^m$ 29.57$^s$ | −71° 26′ 10.3″ | 6.34 | 0.08 | 583 | K2/K3III | |
| HD 74148 | | | 74148 | 42440 | 08$^h$ 39$^m$ 13.24$^s$ | −60° 19′ 02.4″ | 6.35 | 0.71 | 437 | A0V | |
| HD 89805 | | | 89805 | 50562 | 10$^h$ 19$^m$ 42.04$^s$ | −65° 08′ 14.1″ | 6.35 | −2.59 | 2000 | K2II | |
| WR 22 | | V429 | 92740 | 52308 | 10$^h$ 41$^m$ 17.52$^s$ | −59° 40′ 36.9″ | 6.35 | −4.72 | 5344 | WN7 + A(SB1) | Wolf–Rayet star and Algol variable, V$_{max}$ = 6.33$^m$, V$_{min}$ = 6.52$^m$, P = 80.34 d; one of the most luminous stars known |
| HD 93739 | | | 93739 | 52785 | 10$^h$ 47$^m$ 30.62$^s$ | −69° 26′ 15.8″ | 6.35 | −1.57 | 1249 | B2IV | |
| HD 65189 | | | 65189 | 38667 | 07$^h$ 55$^m$ 00.44$^s$ | −52° 35′ 00.1″ | 6.36 | −1.08 | 1003 | B8III | |
| HD 72322 | | | 72322 | 41653 | 08$^h$ 29$^m$ 36.40$^s$ | −55° 11′ 27.3″ | 6.36 | −0.36 | 721 | G0V | |
| V473 Car | | V473 | 76640 | 43763 | 08$^h$ 54$^m$ 54.05$^s$ | −58° 14′ 22.9″ | 6.36 | −0.77 | 869 | B5V | 53 Per variable |
| HD 79699 | | | 79699 | 45214 | 09$^h$ 12$^m$ 50.63$^s$ | −60° 55′ 00.5″ | 6.36 | 0.21 | 553 | B9V | |
| HD 78632 | | | 78632 | 44665 | 09$^h$ 06$^m$ 07.61$^s$ | −64° 29′ 59.7″ | 6.37 | 0.08 | 590 | K3III | |
| HD 61394 | | | 61394 | 36977 | 07$^h$ 36$^m$ 01.62$^s$ | −55° 53′ 15.8″ | 6.39 | 0.06 | 601 | K1/K2IIICN. | |
| HD 96568 | | | 96568 | 54289 | 11$^h$ 06$^m$ 24.32$^s$ | −64° 50′ 23.8″ | 6.39 | 0.58 | 473 | A3V | |
| HD 44267 | | | 44267 | 29913 | 06$^h$ 17$^m$ 51.74$^s$ | −52° 43′ 58.9″ | 6.40 | −0.70 | 858 | K2/K3III | variable star, ΔV = 0.008$^m$, P = 1.32 d |
| HD 62758 | | | 62758 | 37530 | 07$^h$ 42$^m$ 10.22$^s$ | −58° 37′ 51.4″ | 6.40 | −1.18 | 1069 | B2.5V | |
| V368 Car | | V368 | 88647 | 49926 | 10$^h$ 11$^m$ 35.49$^s$ | −58° 49′ 40.2″ | 6.40 | | 801 | M3III | semiregular variable, V$_{max}$ = 6.1$^m$, V$_{min}$ = 6.4$^m$ |
| HD 51210 | | | 51210 | 33012 | 06$^h$ 52$^m$ 45.44$^s$ | −59° 20′ 28.6″ | 6.41 | 0.62 | 470 | A3m... | |
| HD 87438 | | | 87438 | 49223 | 10$^h$ 02$^m$ 49.42$^s$ | −62° 09′ 24.0″ | 6.41 | −3.23 | 2763 | K3Ib | irregular variable, V$_{max}$ = 6.38$^m$, V$_{min}$ = 6.43$^m$ |
| HD 91270 | | | 91270 | 51461 | 10$^h$ 30$^m$ 39.24$^s$ | −61° 21′ 23.4″ | 6.41 | −0.57 | 811 | M2III | suspected variable |
| HD 84046 | | | 84046 | 47422 | 09$^h$ 39$^m$ 45.15$^s$ | −62° 56′ 34.7″ | 6.42 | 0.01 | 623 | B8/B9III/IVw... | suspected variable, V$_{max}$ = 6.42$^m$, V$_{min}$ = 6.8$^m$ |
| HD 88907 | | | 88907 | 50067 | 10$^h$ 13$^m$ 21.20$^s$ | −61° 39′ 31.8″ | 6.42 | −1.06 | 1022 | B2V | |
| V507 Car | | V507 | 90966 | 51265 | 10$^h$ 28$^m$ 18.28$^s$ | −63° 09′ 52.5″ | 6.42 | −2.56 | 2037 | B2/B3III:ne | Be star |
| HD 91094 | | | 91094 | 51327 | 10$^h$ 29$^m$ 03.67$^s$ | −65° 10′ 34.8″ | 6.42 | 0.00 | 627 | M1III | semiregular variable |
| HD 98025 | | | 98025 | 55003 | 11$^h$ 15$^m$ 42.76$^s$ | −57° 21′ 21.1″ | 6.42 | 0.16 | 583 | A3V | |
| HD 78293 | | | 78293 | 44565 | 09$^h$ 04$^m$ 48.00$^s$ | −57° 51′ 09.5″ | 6.43 | −1.21 | 1101 | A8III | |
| HD 93359 | | | 93359 | 52537 | 10$^h$ 44$^m$ 32.42$^s$ | −70° 51′ 18.9″ | 6.43 | 1.25 | 354 | A6IV | |
| HD 65867 | | | 65867 | 38963 | 07$^h$ 58$^m$ 21.47$^s$ | −51° 26′ 54.9″ | 6.44 | 0.43 | 518 | A8/A9IV | suspected eclipsing binary |
| V469 Car | | V469 | 72303 | 41644 | 08$^h$ 29$^m$ 29.82$^s$ | −54° 12′ 42.5″ | 6.44 | −0.28 | 720 | Ap Si | α$^2$ CVn variable |
| HD 49705 | | | 49705 | 32477 | 06$^h$ 46$^m$ 41.70$^s$ | −54° 41′ 42.2″ | 6.45 | 0.93 | 414 | G6III | |
| HD 81896 | | | 81896 | 46143 | 09$^h$ 24$^m$ 37.16$^s$ | −70° 04′ 32.8″ | 6.45 | 0.06 | 617 | K1III | |
| V495 Car | | V495 | 88158 | 49642 | 10$^h$ 07$^m$ 56.64$^s$ | −62° 13′ 17.2″ | 6.45 | −0.55 | 817 | Ap Si | α$^2$ CVn variable |
| WR 24 | | | 93131 | 52488 | 10$^h$ 43$^m$ 52.27$^s$ | −60° 07′ 04.0″ | 6.46 | −5.05 | 6520 | WN7 + A | in Collinder 228; Wolf–Rayet star, V$_{max}$ = 6.46$^m$, V$_{min}$ = 6.49$^m$, P = 4.76 d; one of the most luminous stars known |
| HD 52622 | | | 52622 | 33577 | 06$^h$ 58$^m$ 36.39$^s$ | −56° 23′ 41.2″ | 6.46 | 1.46 | 326 | F2II | suspected variable |
| HD 54967 | | | 54967 | 34350 | 07$^h$ 07$^m$ 16.28$^s$ | −59° 42′ 59.2″ | 6.46 | −1.79 | 1455 | B3V | |
| HD 93738 | | | 93738 | 52815 | 10$^h$ 47$^m$ 53.55$^s$ | −64° 15′ 46.3″ | 6.46 | 0.67 | 469 | B9.5V | in IC 2602 |
| HD 49219 | | | 49219 | 32269 | 06$^h$ 44$^m$ 12.81$^s$ | −54° 41′ 43.9″ | 6.47 | −0.30 | 736 | B5/B6V | variable star, ΔV = 0.011$^m$, P = 1.60 d |
| HD 70267 | | | 70267 | 40655 | 08$^h$ 17$^m$ 55.79$^s$ | −59° 10′ 00.3″ | 6.47 | 2.01 | 254 | F5V | |
| V487 Car | | V487 | 84809 | 47893 | 09$^h$ 45$^m$ 40.64$^s$ | −57° 11′ 09.8″ | 6.47 | −0.66 | 869 | B8III/IV | α$^2$ CVn variable |
| HD 93695 | | | 93695 | 52806 | 10$^h$ 47$^m$ 44.34$^s$ | −59° 52′ 30.9″ | 6.47 | −1.41 | 1230 | B5Vvar | |
| HD 95122 | | | 95122 | 53556 | 10$^h$ 57$^m$ 20.22$^s$ | −69° 02′ 17.0″ | 6.48 | −0.55 | 832 | B7V | suspected variable |
| HD 92399 | | | 92399 | 52103 | 10$^h$ 38$^m$ 45.39$^s$ | −59° 15′ 44.7″ | 6.50 | −1.82 | 1502 | B4/B5III/IV | |
| HD 96248 | | V414 | 96248 | 54179 | 11$^h$ 04$^m$ 57.57$^s$ | −59° 51′ 32.0″ | 6.58 | | 3700 | B1Iab | α Cyg variable, V$_{max}$ = 6.53$^m$, V$_{min}$ = 6.62$^m$, P = 8.52 d |
| HD 57853 | | | 57853 | 35564 | 07$^h$ 20$^m$ 21.43$^s$ | −52° 18′ 31.91″ | 6.63 | | 113 | F9V | component of the HIP 35564 system |
| QX Car | | QX | 86118 | 48589 | 09$^h$ 54$^m$ 33.88$^s$ | −58° 25′ 16.6″ | 6.64 | | 1610 | B2V | Algol variable, V$_{max}$ = 6.6$^m$, V$_{min}$ = 7.21$^m$, P = 4.48 d |
| HD 96446 | | V430 | 96446 | 54266 | 11$^h$ 06$^m$ 05.82$^s$ | −59° 56′ 59.6″ | 6.68 | | 1540 | B2k | β Cep variable, ΔV = 0.03$^m$ |
| HD 53143 | | | 53143 | 33690 | 06$^h$ 59$^m$ 59.66$^s$ | −61° 20′ 10.3″ | 6.68 | | 59.74 | G9V | has a circumstellar disk |
| VY Car | | VY | 93203 | 52538 | 10$^h$ 44$^m$ 32.69$^s$ | −57° 33′ 55.3″ | 6.91 | | 9100 | F7Iab/Ib | classical Cepheid, V$_{max}$ = 6.91$^m$, V$_{min}$ = 8.00$^m$, P = 18.89 d |
| AG Car | | AG | 94910 | 53461 | 10$^h$ 56$^m$ 11.58$^s$ | −60° 27′ 12.8″ | 6.96 | | 17000 | B2-3Ib/WN11 | luminous blue variable, V$_{max}$ = 5.7$^m$, V$_{min}$ = 8.3$^m$, P = 371.4 d |
| BO Car | | BO | 93420 | | 10$^h$ 45$^m$ 50.63$^s$ | −59° 29′ 19.5″ | 7.18 | | | M4Iab: | semiregular variable, V$_{max}$ = 7.15$^m$, V$_{min}$ = 7.95$^m$, P = 130.7 d |
| HD 93403 | | | 93403 | 52628 | 10$^h$ 45$^m$ 44.12$^s$ | −59° 24′ 28.1″ | 7.30 | | 2670 | O5.5I+O7V | binary star |
| HD 93129A | | | 93129A | | 10$^h$ 43$^m$ 57.46$^s$ | −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$^h$ 28$^m$ 43.70$^s$ | −60° 07′ 21.3″ | 7.31 | | 5600 | G2Iab: | classical Cepheid, V$_{max}$ = 7.08$^m$, V$_{min}$ = 7.82$^m$, P = 6.70 d |
| HD 93843 | | | 93843 | | 10$^h$ 48$^m$ 37.78$^s$ | −60° 13′ 25.5″ | 7.33 | | | O5III(f)v | irregular variable, V$_{max}$ = 7.31$^m$, V$_{min}$ = 7.35$^m$ |
| HD 95086 | | | 95086 | 53524 | 10$^h$ 57$^m$ 03.0$^s$ | −68° 40′ 02″ | 7.36 | | 295 | A8III | has a planet (b) |
| HD 93250 | | | 93250 | 52558 | 10$^h$ 44$^m$ 45.03$^s$ | −59° 33′ 54.7″ | 7.50 | | 7500 | O4IIIfc | in Trumpler 16; suspected variable |
| HR Car | | HR | 90177 | 50843 | 10$^h$ 22$^m$ 53.84$^s$ | −59° 37′ 28.4″ | 7.57 | | 17700 | B3Iaep | luminous blue variable, V$_{max}$ = 6.8$^m$, V$_{min}$ = 8.80$^m$ |
| WR 40 | | V385 | 96548 | 54283 | 11$^h$ 06$^m$ 17.20$^s$ | −65° 30′ 35.2″ | 7.70 | | 5900 | WN8h | Wolf–Rayet star and rotating ellipsoidal variable, ΔV = 0.04$^m$, P = 4.76 d; one of the most luminous stars known |
| HD 93205 | | V560 | 93205 | | 10$^h$ 44$^m$ 33.74$^s$ | −59° 44′ 15.5″ | 7.75 | | 7500 | O3.5V((f+)) | in Trumpler 16; rotating ellipsoidal variable, V$_{max}$ = 7.74$^m$, V$_{min}$ = 7.76$^m$, P = 6.08 d |
| IW Car | | IW | 82084 82085 | | 09$^h$ 26$^m$ 53.30$^s$ | −63° 37′ 48.9″ | 7.90 | | | A4Iab/II: | RV Tau variable, V$_{max}$ = 7.77$^m$, V$_{min}$ = 9.10$^m$, P = 143.6 d |
| HD 65216 | | | 65216 | 38558 | 07$^h$ 53$^m$ 41.3$^s$ | −63° 38′ 50.4″ | 7.98 | | 112 | G5V | has two planets (b & c) |
| HD 97152 | | V431 | 97152 | 54574 | 11$^h$ 10$^m$ 04.08$^s$ | −60° 58′ 45.0″ | 8.07 | | 4000 | WC7+O7V | Wolf–Rayet star; eclipsing binary, V$_{max}$ = 7.97$^m$, V$_{min}$ = 8.08$^m$, P = 1.62 d |
| HD 63765 | | | 63765 | 38041 | 07$^h$ 47$^m$ 49.72$^s$ | −54° 15′ 50.9″ | 8.10 | 5.53 | 106 | G9V | Tapecue; has a planet (b) |
| Y Car | | Y | 91565 | 51653 | 10$^h$ 33$^m$ 10.85$^s$ | −58° 29′ 55.1″ | 8.16 | | 3050 | F2 | double-mode Cepheid, V$_{max}$ = 7.53$^m$, V$_{min}$ = 8.48$^m$, P = 3.64 d |
| HD 51608 | | | 51608 | 33229 | 06$^h$ 54$^m$ 51$^s$ | −55° 15′ 34″ | 8.17 | | 114 | K0IV | has two planets (b & c) |
| HD 85628 A | | | 85628 | | 09$^h$ 50$^m$ 19.2$^s$ | −66° 06′ 50″ | 8.19 | | 559 | A3V | has a planet (b) |
| YZ Car | | YZ | 90912 | 51262 | 10$^h$ 28$^m$ 16.85$^s$ | −59° 21′ 00.7″ | 8.24 | | 5900 | G5 | classical Cepheid, V$_{max}$ = 8.24$^m$, V$_{min}$ = 9.08$^m$, P = 18.17 d |
| WR 16 | | V396 | 86161 | 48617 | 09$^h$ 54$^m$ 52.90$^s$ | −57° 43′ 38.3″ | 8.32 | | | WN8h | rotating ellipsoidal variable, ΔV = 0.06$^m$; one of the most luminous stars known |
| EM Car | | EM | 97484 | | 11$^h$ 12$^m$ 04.51$^s$ | −61° 05′ 42.9″ | 8.52 | | | O8V | Algol variable |
| RT Car | | RT | 303310 | 52562 | 10$^h$ 44$^m$ 47.15$^s$ | −59° 24′ 48.1″ | 8.55 | | 1430 | M2Iab: | possibly in Trumpler 15; irregular variable, V$_{max}$ = 8.2$^m$, V$_{min}$ = 9.9$^m$, one of the largest stars known |
| HD 85567 | | V596 | 85567 | 48269 | 09$^h$ 50$^m$ 28.54$^s$ | −60° 58′ 03.0″ | 8.57 | | 6900 | B2 | FS CMa variable, V$_{max}$ = 8.44$^m$, V$_{min}$ = 8.75$^m$ |
| UX Car | | UX | 91039 | 51338 | 10$^h$ 29$^m$ 11.24$^s$ | −57° 36′ 48.3″ | 8.62 | | 2530 | F2II | classical Cepheid, V$_{max}$ = 7.81$^m$, V$_{min}$ = 8.67$^m$, P = 3.68 d |
| XZ Car | | XZ | 305996 | 54101 | 11$^h$ 04$^m$ 13.47$^s$ | −60° 58′ 47.7″ | 8.67 | | | B2:pe | classical Cepheid, V$_{max}$ = 8.05$^m$, V$_{min}$ = 9.12$^m$, P = 16.65 d |
| GG Car | | GG | 94878 | 53444 | 10$^h$ 55$^m$ 58.92$^s$ | −60° 23′ 33.4″ | 8.70 | | | B0/2eq | Be star and re-radiating binary system, V$_{max}$ = 8.44$^m$, V$_{min}$ = 9.08$^m$, P = 31.03 d |
| V403 Car | | V403 | | | 10$^h$ 35$^m$ 40.67$^s$ | −58° 12′ 44.6″ | 8.74 | | 8400 | B1III | in NGC 3293; β Cep variable, ΔV = 0.033$^m$, P = 0.25 d |
| Tr 16-104 | | V572 | | | 10$^h$ 44$^m$ 47.31$^s$ | −59° 43′ 53.2″ | 8.75 | | 7500 | O7V((f))+ O9.5V+ B0.2IV | in Trumpler 16; Algol variable, V$_{max}$ = 8.66$^m$, V$_{min}$ = 9.07$^m$, P = 2.15 d |
| V348 Car | | V348 | 90707 | | 10$^h$ 29$^m$ 59.00$^s$ | −57° 40′ 32.8″ | 8.78 | | | B1III | β Lyr variable, V$_{max}$ = 8.55$^m$, V$_{min}$ = 8.93$^m$, P = 5.56 d |
| WR 25 | | | 93162 | | 10$^h$ 44$^m$ 10.34$^s$ | −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$^h$ 30$^m$ 56.99$^s$ | −57° 59′ 28.2″ | 8.89 | | 739 | Ap... | rapidly oscillating Ap star |
| WR 23 | | | 92809 | 52331 | 10$^h$ 41$^m$ 38.32$^s$ | −58° 46′ 18.7″ | 9.03 | | 3400 | WC6 | Wolf–Rayet star |
| HD 92024 | | V381 | 92024 | | 10$^h$ 36$^m$ 08.31$^s$ | −58° 13′ 04.77″ | 9.04 | | 8400 | B1III | in NGC 3293; β Cep variable, V$_{max}$ = 9.04$^m$, V$_{min}$ = 9.06$^m$, P = 0.17 d |
| GH Car | | GH | 306077 | 54621 | 11$^h$ 10$^m$ 44.59$^s$ | −60° 45′ 01.0″ | 9.20 | | | G0 | classical Cepheid, V$_{max}$ = 9$^m$, V$_{min}$ = 9.35$^m$, P = 5.73 d |
| WZ Car | | WZ | 94777 | 53397 | 10$^h$ 55$^m$ 18.73$^s$ | −60° 56′ 24.0″ | 9.37 | | 4700 | F8 | classical Cepheid, V$_{max}$ = 8.63$^m$, V$_{min}$ = 9.88$^m$, P = 23.02 d |
| CPD -59° 2635 | | V731 | | | 10$^h$ 45$^m$ 12.72$^s$ | −59° 44′ 46.2″ | 9.43 | | 7500 | O8V+O9.5V | in Trumpler 16; Algol variable, V$_{max}$ = 9.27$^m$, V$_{min}$ = 9.78$^m$, P = 2.30 d |
| Gliese 341 | | | 304636 | 45908 | 09$^h$ 21$^m$ 37.602$^s$ | −60° 16′ 55.03″ | 9.465 | | 34 | M1V | has a planet (b) |
| V392 Car | | V392 | | | 07$^h$ 58$^m$ 10.47$^s$ | −60° 51′ 57.5″ | 9.49 | | | A2Vp... | in NGC 2516; Algol and α$^2$ CVn variable, V$_{max}$ = 9.49$^m$, V$_{min}$ = 9.67$^m$ |
| XY Car | | XY | 308149 | 53945 | 11$^h$ 02$^m$ 16.07$^s$ | −64° 15′ 46.5″ | 9.49 | | | G5 | classical Cepheid, V$_{max}$ = 8.82$^m$, V$_{min}$ = 9.77$^m$, P = 12.43 d |
| HD 87643 | | V640 | 87643 | | 10$^h$ 04$^m$ 30.29$^s$ | −58° 39′ 52.1″ | 9.50 | | | B2e | Orion variable, V$_{max}$ = 7.4$^m$, V$_{min}$ = 9.8$^m$ |
| CPD -59 2628 | | V573 | | | 10$^h$ 45$^m$ 08.23$^s$ | −59° 40′ 49.5″ | 9.52 | | 7500 | O9.5V+B0.3V | in Trumpler 16; Algol variable |
| HD 90657 | | V398 | 90657 | 51109 | 10$^h$ 26$^m$ 31.41$^s$ | −58° 38′ 26.2″ | 9.69 | | 3500 | WN5+O4-6 | Wolf–Rayet star; eclipsing binary, ΔV = 0.035$^m$ |
| GL Car | | GL | 306168 | | 11$^h$ 14$^m$ 39.84$^s$ | −60° 39′ 36.3″ | 9.70 | | | B3:V | Algol variable |
| DW Car | | DW | 305543 | | 10$^h$ 43$^m$ 10.07$^s$ | −60° 02′ 11.7″ | 9.85 | | | B2:pe | in Collinder 228; Algol variable |
| SS73 17 | | V648 | | | 10$^h$ 11$^m$ 02.95$^s$ | −57° 48′ 13.9″ | 9.99 | | | M3pe+OB | Z And variable, V$_{max}$ = 9.6$^m$, V$_{min}$ = 10.0$^m$, P = 520 d |
| CPD -57 2874 | | | | | 10$^h$ 15$^m$ 21.97$^s$ | −57° 51′ 42.7″ | 10.16 | | | sgB1[e] | B[e] star |
| GZ Car | | GZ | 302719 | 50615 | 10$^h$ 20$^m$ 20.37$^s$ | −59° 22′ 35.8″ | 10.20 | | 2400 | G5 | double-mode Cepheid, V$_{max}$ = 9.98$^m$, V$_{min}$ = 10.47$^m$, P = 4.16 d |
| HH Car | | HH | 303503 | | 10$^h$ 53$^m$ 36.47$^s$ | −59° 27′ 18.2″ | 10.31 | | | B | Algol variable, V$_{max}$ = 10.3$^m$, V$_{min}$ = 10.82$^m$, P = 3.23 d |
| EY Car | | EY | | 52380 | 10$^h$ 42$^m$ 23.03$^s$ | −61° 09′ 57.3″ | 10.35 | | | B2:pe | double-mode Cepheid, V$_{max}$ = 10.01$^m$, V$_{min}$ = 10.56$^m$, P = 2.88 d |
| HD 307938 | | V557 | 307938 | | 10$^h$ 42$^m$ 41.52$^s$ | −64° 21′ 04.4″ | 10.57 | | | G2V | BY Dra variable, ΔV = 0.21$^m$ |
| WR 18 | | V500 | 89358 | 50368 | 10$^h$ 17$^m$ 02.27$^s$ | −57° 54′ 47.9″ | 10.6 | | 6300 | WN4-s | Wolf–Rayet star |
| HD 94546 | | V428 | 94546 | 53274 | 10$^h$ 53$^m$ 44.82$^s$ | −59° 30′ 46.7″ | 10.7 | | | WN4+O8V | Wolf–Rayet star; eclipsing binary, ΔV = 0.05$^m$ |
| He 3-519 | | | | | 10$^h$ 53$^m$ 59.59$^s$ | −60° 26′ 44.3″ | 10.85 | | | WN11 | Wolf–Rayet star, V$_{max}$ = 10.6$^m$, V$_{min}$ = 11.0$^m$ |
| NGC 3603-A1 | | | 97950A | | 11$^h$ 15$^m$ 07.31$^s$ | −61° 15′ 38.4″ | 11.12 | | 20000 | WN6ha+O3V | in NGC 3603; Algol variable, ΔV = 0.45$^m$, P = 3.77 d both components among the most luminous and massive stars known |
| CR Car | | CR | | | 10$^h$ 32$^m$ 54.07$^s$ | −58° 31′ 15.5″ | 11.30 | | | B2:pe | classical Cepheid, V$_{max}$ = 11.3$^m$, V$_{min}$ = 11.89$^m$, P = 9.76 d |
| NGC 3603-B | | | 97950B | | 11$^h$ 15$^m$ 07.41$^s$ | −61° 15′ 38.6″ | 11.33 | | | WN6h+abs | one of the most luminous and most massive stars known |
| Innes' star | | | | | 11$^h$ 16$^m$ 00.21$^s$ | −57° 32′ 51.6″ | 11.52 | | 41.31 | M3.5 | has a planet |
| QU Car | | QU | 310376 | 54226 | 11$^h$ 05$^m$ 42.49$^s$ | −68° 37′ 58.2″ | 11.54 | | 1290 | B+... | V Sge variable, V$_{max}$ = 10.9$^m$, V$_{min}$ = 11.7$^m$, P = 0.45 d |
| WR 30 | | V541 | 94305 | | 10$^h$ 51$^m$ 06.01$^s$ | −62° 17′ 01.7″ | 11.73 | | | WC6+O7.5V | Algol variable, ΔV = 0.09$^m$ |
| Wray 15-751 | | V432 | | | 11$^h$ 08$^m$ 40.06$^s$ | −60° 42′ 51.7″ | 11.79 | | | WR: | luminous blue variable, V$_{max}$ = 10.7$^m$, V$_{min}$ = 12.43$^m$ |
| NGC 3603-C | | | 97950C | | 11$^h$ 15$^m$ 07.59$^s$ | −61° 15′ 18.0″ | 11.89 | | | WN6h+abs | spectroscopic binary |
| FO 15 | | V662 | | | 10$^h$ 45$^m$ 36.32$^s$ | −59° 48′ 23.2″ | 12.09 | | 7500 | O5.5V+O9.5V | in Trumpler 16; Algol variable, V$_{max}$ = 12.09$^m$, V$_{min}$ = 12.7$^m$, P = 1.41 d |
| Sher 25 | | | | | 11$^h$ 15$^m$ 07.8$^s$ | −61° 15′ 17″ | 12.27 | | | B1.5Iab | in NGC 3603; potential supernova progenitor |
| WR 30a | | V574 | | | 10$^h$ 51$^m$ 38.93$^s$ | −60° 56′ 35.2″ | 12.73 | | | WR+... | Algol variable, ΔV = 0.05$^m$ |
| GJ 1128 | | | | | 09$^h$ 42$^m$ 46.356$^s$ | −68° 53′ 06.04″ | 12.78 | | | M4.0V | |
| He 2-38 | | V366 | | | 09$^h$ 54$^m$ 43.29$^s$ | −57° 18′ 52.4″ | 12.92 | | | M5-7.5 | Mira and Z And variable, V$_{max}$ = 12.1$^m$, V$_{min}$ = 14.4$^m$, P = 433 d |
| BPM 6502 | | V727 | | | 10$^h$ 44$^m$ 10.23$^s$ | −69° 18′ 18.0″ | 13.09 | | | DA2.2+M | re-radiating binary system |
| WR 20a | | V712 | | | 10$^h$ 23$^m$ 58.00$^s$ | −57° 45′ 49.0″ | 13.5 | | | O3If*/WN6+ O3If*/WN6 | in Westerlund 2; Algol variable |
| LHS 288 | | | | | 10$^h$ 44$^m$ 21.32$^s$ | −61° 12′ 38.4″ | 13.92 | | 15.602 | M4 | |
| OGLE-TR-113 | | V752 | | | 10$^h$ 52$^m$ 24.4$^s$ | −61° 26′ 48.5″ | 14.42 | | 1800 | K | has a transiting planet (b) |
| MTT 68 | | | | | 11$^h$ 14$^m$ 59.50$^s$ | −61° 14′ 33.89″ | 14.72 | −6.4 | 25,000 | O2If* | rare O2If* type, along with HD 93129A |
| 2S 0921-630 | | V395 | | | 09$^h$ 22$^m$ 35.20$^s$ | −63° 17′ 38.5″ | 15.3 | | | K0IIIe | low-mass X-ray binary |
| OGLE-TR-123 | | V816 | | | 11$^h$ 06$^m$ 51.1$^s$ | −61° 11′ 10.5″ | 15.47 | | | FV+MV | possibly has a transiting planet |
| OGLE-TR-111 | | V759 | | | 10$^h$ 53$^m$ 17.9$^s$ | −61° 24′ 20.3″ | 15.55 | | 5000 | G | has a transiting planet (b) and a possible second planet |
| OGLE-TR-132 | | V742 | | | 10$^h$ 50$^m$ 34.7$^s$ | −61° 57′ 25.9″ | 15.72 | | 7110 | F | has a transiting planet (b) |
| OY Car | | OY | | | 10$^h$ 06$^m$ 22.07$^s$ | −70° 14′ 04.6″ | 16.2 | | 277 | M5/M6:... | SU UMa variable and eclipsing binary, V$_{max}$ = 11.2$^m$, V$_{min}$ = 16.2$^m$, P = 0.063 d |
| OGLE-TR-182 | | | | | 11$^h$ 09$^m$ 18.73$^s$ | −61° 05′ 42.93″ | 16.84 | | 12700 | G | has a transiting planet (b) |
| OGLE-TR-211 | | | | | 10$^h$ 40$^m$ 14.39$^s$ | −62° 27′ 20.2″ | | | 5300 | F | has a transiting planet (b) |
| OGLE-TR-122 | | V817 | | | 11$^h$ 06$^m$ 52.0$^s$ | −60° 51′ 45.7″ | | | | | has a transiting brown dwarf |
| OGLE2-TR-L9 | | | | | 11$^h$ 07$^m$ 55$^s$ | −61° 08′ 46″ | | | 2935 | F3 | has a transiting planet (b) |
| 1E 1048.1-5937 | | | | | 10$^h$ 50$^m$ 08.93$^s$ | −59° 53′ 19.9″ | | | | Be | anomalous X-ray pulsar |
| DENIS J081730.0-615520 | | | | | 08$^h$ 17$^m$ 30.01$^s$ | −61° 55′ 15.8″ | | | 16.1 | T6 | brown dwarf |
| PSR J1048-5832 | | | | | 10$^h$ 48$^m$ 12.20$^s$ | −58° 32′ 05.8″ | | | | | pulsar |
| PSR J1119-6127 | | | | | 11$^h$ 19$^m$ 14.30$^s$ | −61° 27′ 49.5″ | | | | | pulsar |
| Table legend:  • Name = Proper name  • B = Bayer designation  • F or/and G. = Flamsteed designation or Gould designation  • Var = Variable star designation  • HD = Henry Draper Catalogue designation number  • HIP = Hipparcos Catalogue designation number  • RA = Right ascension for the Epoch/Equinox J2000.0  • Dec = Declination for the Epoch/Equinox J2000.0  • vis. mag. = visual magnitude (m or m$_v$), also known as apparent magnitude  • abs. mag. = absolute magnitude (M$_v$)  • Dist. (ly) = Distance in light-years from Earth  • Sp. class = Spectral class of the star in the stellar classification system  • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] ||||||||||||