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List of stars in Carina

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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 23 57.09 −52° 41′ 44.6″ −0.72 −5.53 313 A9 II Suhel; 2nd brightest star
β Car β 80007 45238 09 13 12.24 −69° 43′ 02.9″ 1.67 −0.99 111 A1 III 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, Vmax = 1.82, Vmin = 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, Vmax = 2.23, Vmin = 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, Vmax = 3.22, Vmin = 3.55
V337 Car q V337 89388 50371 10 17 05.01 −61° 19′ 56.4″ 3.39 −3.38 736 K3II irregular variable, Vmax = 3.36, Vmin = 3.44
a Car a V357 79351 45080 09 10 58.11 −58° 58′ 00.9″ 3.43 −2.11 418 B2IV eclipsing binary, Vmax = 3.41, Vmin = 3.44
χ Car χ 65575 38827 07 56 46.74 −52° 58′ 56.6″ 3.46 −1.91 387 B3IVp β Cep variable, ΔV = 0.015, P = 0.10 d
l Car l 84810 47854 09 45 14.83 −62° 30′ 28.5″ 3.69 −4.64 1509 G5Iab/Ib classical Cepheid, Vmax = 3.28, Vmin = 4.18, P = 35.54 d
HD 94510 u 94510 53253 10 53 29.57 −58° 51′ 11.8″ 3.78 1.42 97 K0III-IV... suspected variable, Vmax = 3.75, Vmin = 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, Vmax = 3.77, Vmin = 4.05
HD 79447 i 79447 45101 09 11 16.77 −62° 19′ 01.3″ 3.96 −1.97 499 B3IV variable star, ΔV = 0.008, P = 22.26 d
HD 90589 I 90589 50954 10 24 23.74 −74° 01′ 53.6″ 3.99 2.94 53 F2IV suspected variable, Vmax = 3.96, Vmin = 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 suspected variable, Vmax = 4.31, Vmin = 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, ΔV = 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 Foramen, Tseen She; in Trumpler 16; binary star; luminous blue variable, Vmax = −0.8, Vmin = 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, Vmax = 4.40, Vmin = 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, Vmax = 4.50, Vmin = 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 z 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, Vmax = 4.63, Vmin = 4.72, P = 88.3 d
V345 Car E V345 78764 44626 09 05 38.38 −70° 32′ 18.7″ 4.67 −2.94 1079 B2IVe γ Cas variable, Vmax = 4.67, Vmin = 4.78, P = 137.7 d
HD 92397 t 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, Vmax = 4.79, Vmin = 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 e 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 b V376 77002 43937 08 56 58.43 −59° 13′ 45.7″ 4.93 −1.47 621 B2IV-V β Cep variable, Vmax = 4.91, Vmin = 4.96, P = 0.021 d
HD 91496 91496 51495 10 31 02.07 −73° 13′ 17.4″ 4.94 −2.42 964 K4/K5III suspected variable, Vmax = 4.87, Vmin = 4.97
HD 90264 L 90264 50847 10 22 58.18 −66° 54′ 05.5″ 4.97 −0.63 430 B8V
HD 92063 t 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 z V371 96919 54461 11 08 34.01 −61° 56′ 49.8″ 5.12 −6.03 5525 B9Ia α Cyg variable, Vmax = 5.12, Vmin = 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: α CVn variable, ΔV = 0.026, P = 3.28 d
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 b 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, Vmax = 5.15, Vmin = 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 e 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, Vmax = 5.32, Vmin = 5.43, P = 14.68 d
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, Vmax = 5.45, Vmin = 5.52, P = 1.33 d
V450 Car V450 53921 34000 07 03 15.11 −59° 10′ 41.3″ 5.50 −0.35 482 B9IV 53 Per variable, ΔV = 0.02
HD 92664 V364 92664 52221 10 40 11.46 −65° 06′ 00.9″ 5.51 −0.26 466 B9p Si α CVn variable, Vmax = 5.48, Vmin = 5.52, P = 1.67 d
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 variable star, ΔV = 0.004, P = 1.74 d
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, ΔV = 0.027, P = 0.12 d
HD 88661 QY 88661 49934 10 11 46.47 −58° 03′ 38.0″ 5.70 −2.29 1294 B2IVnpe γ Cas variable, Vmax = 5.63, Vmin = 5.83
S Car S 88366 49751 10 09 22.01 −61° 32′ 57.1″ 5.71 1780 K5-M6e Mira variable, Vmax = 4.5, Vmin = 9.9, P = 149.49 d
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 suspected eclipsing binary, ΔV = 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, Vmax = 5.72, Vmin = 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 rotating ellipsoidal variable, Vmax = 5.88, Vmin = 5.92, P = 2.90 d
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 variable star, ΔV = 0.008, P = 1.56 d
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... α CVn variable, ΔV = 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 variable star, ΔV = 0.005, P = 0.084 d
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, Vmax = 3.9, Vmin = 10.5, P = 308.71 d
HD 91619 V369 91619 51676 10 33 25.40 −58° 11′ 24.6″ 6.11 −6.99 13583 B7Ia α Cyg variable, ΔV = 0.1, P = 1.12 d
U Car U 95109 53589 10 57 48.19 −59° 43′ 55.9″ 6.11 G3Ia classical Cepheid, Vmax = 5.74, Vmin = 6.96, P = 38.83 d
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, Vmax = 6.19, Vmin = 6.36, P = 16.93 d
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 semiregular variable, Vmax = 6.2, Vmin = 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, ΔV = 0.04, P = 1.02 d
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 suspected variable, Vmax = 6.28, Vmin = 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, Vmax = 6.16, Vmin = 6.49, P = 6.00 d
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 suspected variable, Vmax = 6.33, Vmin = 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, Vmax = 6.33, Vmin = 6.52, P = 80.34 d; 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 variable star, ΔV = 0.008, P = 1.32 d
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 semiregular variable, Vmax = 6.1, Vmin = 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 irregular variable, Vmax = 6.38, Vmin = 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... suspected variable, Vmax = 6.42, Vmin = 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 α 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 α 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, Vmax = 6.46, Vmin = 6.49, P = 4.76 d; 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 variable star, ΔV = 0.011, P = 1.60 d
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 α 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, Vmax = 6.53, Vmin = 6.62, P = 8.52 d
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, Vmax = 6.6, Vmin = 7.21, P = 4.48 d
HD 96446 V430 96446 54266 11 06 05.82 −59° 56′ 59.6″ 6.68 1540 B2k β Cep variable, ΔV = 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, Vmax = 6.91, Vmin = 8.00, P = 18.89 d
AG Car AG 94910 53461 10 56 11.58 −60° 27′ 12.8″ 6.96 17000 B2-3Ib/WN11 luminous blue variable, Vmax = 5.7, Vmin = 8.3, P = 371.4 d
BO Car BO 93420 10 45 50.63 −59° 29′ 19.5″ 7.18 M4Iab: semiregular variable, Vmax = 7.15, Vmin = 7.95, P = 130.7 d
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, Vmax = 7.08, Vmin = 7.82, P = 6.70 d
HD 93843 93843 10 48 37.78 −60° 13′ 25.5″ 7.33 O5III(f)v irregular variable, Vmax = 7.31, Vmin = 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, Vmax = 6.8, Vmin = 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, ΔV = 0.04, P = 4.76 d; 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, Vmax = 7.74, Vmin = 7.76, P = 6.08 d
IW Car IW 82084
82085
09 26 53.30 −63° 37′ 48.9″ 7.90 A4Iab/II: RV Tau variable, Vmax = 7.77, Vmin = 9.10, P = 143.6 d
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, Vmax = 7.97, Vmin = 8.08, P = 1.62 d
HD 63765 63765 38041 07 47 49.72 −54° 15′ 50.9″ 8.10 5.53 106 G9V Tapecue; has a planet (b)
Y Car Y 91565 51653 10 33 10.85 −58° 29′ 55.1″ 8.16 3050 F2 double-mode Cepheid, Vmax = 7.53, Vmin = 8.48, P = 3.64 d
HD 51608 51608 33229 06 54 51 −55° 15′ 34″ 8.17 114 K0IV has two planets (b & c)
HD 85628 A 85628 09 50 19.2 −66° 06′ 50″ 8.19 559 A3V has a planet (b)
YZ Car YZ 90912 51262 10 28 16.85 −59° 21′ 00.7″ 8.24 5900 G5 classical Cepheid, Vmax = 8.24, Vmin = 9.08, P = 18.17 d
WR 16 V396 86161 48617 09 54 52.90 −57° 43′ 38.3″ 8.32 WN8h rotating ellipsoidal variable, ΔV = 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, Vmax = 8.2, Vmin = 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, Vmax = 8.44, Vmin = 8.75
UX Car UX 91039 51338 10 29 11.24 −57° 36′ 48.3″ 8.62 2530 F2II classical Cepheid, Vmax = 7.81, Vmin = 8.67, P = 3.68 d
XZ Car XZ 305996 54101 11 04 13.47 −60° 58′ 47.7″ 8.67 B2:pe classical Cepheid, Vmax = 8.05, Vmin = 9.12, P = 16.65 d
GG Car GG 94878 53444 10 55 58.92 −60° 23′ 33.4″ 8.70 B0/2eq Be star and re-radiating binary system, Vmax = 8.44, Vmin = 9.08, P = 31.03 d
V403 Car V403 10 35 40.67 −58° 12′ 44.6″ 8.74 8400 B1III in NGC 3293; β Cep variable, ΔV = 0.033, P = 0.25 d
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, Vmax = 8.66, Vmin = 9.07, P = 2.15 d
V348 Car V348 90707 10 29 59.00 −57° 40′ 32.8″ 8.78 B1III β Lyr variable, Vmax = 8.55, Vmin = 8.93, P = 5.56 d
WR 25 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, Vmax = 9.04, Vmin = 9.06, P = 0.17 d
GH Car GH 306077 54621 11 10 44.59 −60° 45′ 01.0″ 9.20 G0 classical Cepheid, Vmax = 9, Vmin = 9.35, P = 5.73 d
WZ Car WZ 94777 53397 10 55 18.73 −60° 56′ 24.0″ 9.37 4700 F8 classical Cepheid, Vmax = 8.63, Vmin = 9.88, P = 23.02 d
CPD -59° 2635 V731 10 45 12.72 −59° 44′ 46.2″ 9.43 7500 O8V+O9.5V in Trumpler 16; Algol variable, Vmax = 9.27, Vmin = 9.78, P = 2.30 d
V392 Car V392 07 58 10.47 −60° 51′ 57.5″ 9.49 A2Vp... in NGC 2516; Algol and α CVn variable, Vmax = 9.49, Vmin = 9.67
XY Car XY 308149 53945 11 02 16.07 −64° 15′ 46.5″ 9.49 G5 classical Cepheid, Vmax = 8.82, Vmin = 9.77, P = 12.43 d
HD 87643 V640 87643 10 04 30.29 −58° 39′ 52.1″ 9.50 B2e Orion variable, Vmax = 7.4, Vmin = 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, ΔV = 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, Vmax = 9.6, Vmin = 10.0, P = 520 d
CPD -57 2874 10 15 21.97 −57° 51′ 42.7″ 10.16 sgB1 B star
GZ Car GZ 302719 50615 10 20 20.37 −59° 22′ 35.8″ 10.20 2400 G5 double-mode Cepheid, Vmax = 9.98, Vmin = 10.47, P = 4.16 d
HH Car HH 303503 10 53 36.47 −59° 27′ 18.2″ 10.31 B Algol variable, Vmax = 10.3, Vmin = 10.82, P = 3.23 d
EY Car EY 52380 10 42 23.03 −61° 09′ 57.3″ 10.35 B2:pe double-mode Cepheid, Vmax = 10.01, Vmin = 10.56, P = 2.88 d
HD 307938 V557 307938 10 42 41.52 −64° 21′ 04.4″ 10.57 G2V BY Dra variable, ΔV = 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, ΔV = 0.05
He 3-519 10 53 59.59 −60° 26′ 44.3″ 10.85 WN11 Wolf–Rayet star, Vmax = 10.6, Vmin = 11.0
NGC 3603-A1 97950A 11 15 07.31 −61° 15′ 38.4″ 11.12 20000 WN6ha+O3V in NGC 3603; Algol variable, ΔV = 0.45, P = 3.77 d 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, Vmax = 11.3, Vmin = 11.89, P = 9.76 d
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, Vmax = 10.9, Vmin = 11.7, P = 0.45 d
WR 30 V541 94305 10 51 06.01 −62° 17′ 01.7″ 11.73 WC6+O7.5V Algol variable, ΔV = 0.09
Wray 15-751 V432 11 08 40.06 −60° 42′ 51.7″ 11.79 WR: luminous blue variable, Vmax = 10.7, Vmin = 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, Vmax = 12.09, Vmin = 12.7, P = 1.41 d
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, ΔV = 0.05
GJ 1128 09 42 46.356 −68° 53′ 06.04″ 12.78 M4.0V
He 2-38 V366 09 54 43.29 −57° 18′ 52.4″ 12.92 M5-7.5 Mira and Z And variable, Vmax = 12.1, Vmin = 14.4, P = 433 d
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)
MTT 68 11 14 59.50 −61° 14′ 33.89″ 14.72 −6.4 25,000 O2If* rare O2If* type, along with HD 93129A
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, Vmax = 11.2, Vmin = 16.2, P = 0.063 d
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
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 mv), also known as apparent magnitude
 • abs. mag. = absolute magnitude (Mv)
 • 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

See also

Notes

  1. Gray, R. O.; Garrison, R. F. (1989-02-01). "The Early F-Type Stars: Refined Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation". The Astrophysical Journal Supplement Series. 69: 301. Bibcode:1989ApJS...69..301G. doi:10.1086/191315. ISSN 0067-0049.
  2. Lopez-Cruz, O.; Garrison, R. F. (1993-01-01). "A Spectroscopic Study of High Galactic Latitude F Supergiant Stars". Luminous High-Latitude Stars. 45: 59. Bibcode:1993ASPC...45...59L.
  3. Kunitzsch, P., & Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 25. ISBN 978-1-931559-44-7.{{cite book}}: CS1 maint: multiple names: authors list (link)
  4. Gray, R. O.; Corbally, C. J.; Garrison, R. F.; McFadden, M. T.; Bubar, E. J.; McGahee, C. E.; O'Donoghue, A. A.; Knox, E. R. (July 2006). "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. doi:10.1086/504637. ISSN 0004-6256.

References

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