# List of stars in Vela

This is the list of notable stars in the constellation Vela, 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 Vela does not have a full complement of Greek-letter designations. For example, since Argo Navis's alpha star went to Carina, there is no Alpha Velorum.
| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| γ$^2$ Vel | γ$^2$ | | 68273 | 39953 | 08$^h$ 09$^m$ 31.96$^s$ | −47° 20′ 11.8″ | 1.83 | −5.84 | 1120 | WC8 + O7.5III | Suhail, Suhail al Muhlif, Muliphein, Regor; double star; Wolf-Rayet star, V$_{max}$ = 1.81$^m$, V$_{min}$ = 1.87$^m$ |
| δ Vel | δ | | 74956 | 42913 | 08$^h$ 44$^m$ 42.20$^s$ | −54° 42′ 30.8″ | 1.96 | 0.00 | 81 | A1Va(n) | Koo She, Alsephina; quadruple star; Algol variable, ΔV = 0.4$^m$, P = 45.15 d |
| λ Vel | λ | | 78647 | 44816 | 09$^h$ 07$^m$ 59.78$^s$ | −43° 25′ 57.4″ | 2.21 | −3.97 | 573 | K4Ib-II | Suhail, Suhail al Muhlif, Al Suhail, Alsuhail, Suhail Alwazn, Muliphein; semiregular variable, V$_{max}$ = 2.14$^m$, V$_{min}$ = 2.3$^m$ |
| κ Vel | κ | | 81188 | 45941 | 09$^h$ 22$^m$ 06.83$^s$ | −55° 00′ 38.5″ | 2.47 | −3.62 | 539 | B2IV | Markeb; Markab |
| μ Vel | μ | | 93497 | 52727 | 10$^h$ 46$^m$ 46.12$^s$ | −49° 25′ 12.5″ | 2.69 | −0.06 | 116 | G5III SB | |
| HD 82668 | N | | 82668 | 46701 | 09$^h$ 31$^m$ 13.35$^s$ | −57° 02′ 03.8″ | 3.16 | −1.15 | 238 | K5III | semiregular variable, V$_{max}$ = 3.12$^m$, V$_{min}$ = 3.18$^m$ |
| φ Vel | φ | | 86440 | 48774 | 09$^h$ 56$^m$ 51.75$^s$ | −54° 34′ 04.1″ | 3.52 | −5.34 | 1929 | B5Ib | Tseen Ke |
| ο Vel | ο | | 74195 | 42536 | 08$^h$ 40$^m$ 17.61$^s$ | −52° 55′ 19.1″ | 3.60 | −2.31 | 495 | B3IV | in IC 2391; slowly pulsating B star, V$_{max}$ = 3.57$^m$, V$_{min}$ = 3.63$^m$, P = 2.80 d |
| HD 78004 | c | | 78004 | 44511 | 09$^h$ 04$^m$ 09.32$^s$ | −47° 05′ 51.8″ | 3.75 | −1.13 | 309 | K2III | |
| HD 74180 | b | | 74180 | 42570 | 08$^h$ 40$^m$ 37.58$^s$ | −46° 38′ 55.5″ | 3.81 | −7.06 | 4900 | F3Ia | suspected variable, V$_{max}$ = 3.80$^m$, V$_{min}$ = 3.91$^m$ |
| p Vel | p | | 92139 | 51986 | 10$^h$ 37$^m$ 18.26$^s$ | −48° 13′ 32.2″ | 3.84 | 1.72 | 86 | A3m+... | |
| HD 88955 | q | | 88955 | 50191 | 10$^h$ 14$^m$ 44.27$^s$ | −42° 07′ 19.4″ | 3.85 | 1.36 | 103 | A2V | |
| HD 75063 | a | | 75063 | 43023 | 08$^h$ 46$^m$ 01.65$^s$ | −46° 02′ 29.5″ | 3.87 | −4.52 | 1552 | A1III | |
| ψ Vel A | ψ | | 82434A | 46651 | 09$^h$ 30$^m$ 42.11$^s$ | −40° 28′ 00.8″ | 3.91 | 2.57 | 61 | F3VFe-0.7 | |
| HD 74772 | d | | 74772 | 42884 | 08$^h$ 44$^m$ 23.97$^s$ | −42° 38′ 57.6″ | 4.05 | −0.18 | 228 | G5III | |
| HD 73634 | e | | 73634 | 42312 | 08$^h$ 37$^m$ 38.64$^s$ | −42° 59′ 20.8″ | 4.11 | −4.11 | 1436 | A6II | |
| γ$^1$ Vel | γ$^1$ | | 68243 | | 08$^h$ 09$^m$ 29.30$^s$ | −47° 20′ 45.0″ | 4.27 | −3.62 | 840 | B2III | component of the γ Vel system, spectroscopic binary; suspected variable |
| HD 92449 | x | | 92449 | 52154 | 10$^h$ 39$^m$ 18.41$^s$ | −55° 36′ 11.8″ | 4.29 | −2.92 | 901 | G2II | |
| HD 83446 | M | | 83446 | 47175 | 09$^h$ 36$^m$ 49.66$^s$ | −49° 21′ 18.5″ | 4.34 | 1.75 | 107 | A5V | |
| HD 95370 | i | | 95370 | 53773 | 11$^h$ 00$^m$ 09.25$^s$ | −42° 13′ 33.1″ | 4.37 | 0.39 | 204 | A3IV | |
| HD 77258 | w | | 77258 | 44191 | 09$^h$ 00$^m$ 05.44$^s$ | −41° 15′ 13.5″ | 4.47 | 0.52 | 201 | K0III+... | suspected variable |
| MV Vel | J | MV | 89890 | 50676 | 10$^h$ 20$^m$ 54.81$^s$ | −56° 02′ 35.6″ | 4.49 | −3.24 | 1150 | B3III | Be star; ΔV = 0.06$^m$ |
| HD 85622 | m | | 85622 | 48374 | 09$^h$ 51$^m$ 40.69$^s$ | −46° 32′ 51.5″ | 4.58 | −3.03 | 1083 | G5Ib | variable star, ΔV = 0.005$^m$, P = 1.64 d |
| GZ Vel | | GZ | 89682 | 50555 | 10$^h$ 19$^m$ 36.77$^s$ | −55° 01′ 45.5″ | 4.59 | −3.71 | 1489 | K3II | slow irregular variable |
| HD 79940 | k | | 79940 | 45448 | 09$^h$ 15$^m$ 45.07$^s$ | −37° 24′ 47.3″ | 4.63 | 1.10 | 166 | F3/F5V | |
| H Vel | H | | 76805 | 43878 | 08$^h$ 56$^m$ 19.28$^s$ | −52° 43′ 24.6″ | 4.68 | −0.63 | 376 | B5V | |
| HD 74272 | n | | 74272 | 42624 | 08$^h$ 41$^m$ 13.14$^s$ | −47° 19′ 01.7″ | 4.74 | −4.08 | 1895 | A5II | |
| HD 70930 | B | | 70930 | 41039 | 08$^h$ 22$^m$ 31.70$^s$ | −48° 29′ 25.4″ | 4.82 | −3.79 | 1720 | B1V | suspected variable |
| HD 89998 | r | | 89998 | 50799 | 10$^h$ 22$^m$ 19.61$^s$ | −41° 39′ 00.4″ | 4.82 | 0.88 | 200 | K1IIIvar | |
| HY Vel | | HY | 74560 | 42726 | 08$^h$ 42$^m$ 25.41$^s$ | −53° 06′ 50.5″ | 4.83 | −1.01 | 479 | B3IV | in IC 2391; slowly pulsating B star, V$_{max}$ = 4.81$^m$, V$_{min}$ = 4.86$^m$, P = 1.55 d |
| HD 88206 | Q | | 88206 | 49712 | 10$^h$ 08$^m$ 56.25$^s$ | −51° 48′ 40.5″ | 4.85 | −2.76 | 1083 | B3IV | |
| HD 91324 | | | 91324 | 51523 | 10$^h$ 31$^m$ 22.23$^s$ | −53° 42′ 57.6″ | 4.89 | 3.19 | 71 | F6V | |
| HD 79917 | l | | 79917 | 45439 | 09$^h$ 15$^m$ 36.76$^s$ | −38° 34′ 11.7″ | 4.92 | 0.73 | 225 | K1III | |
| HD 75710 | g | | 75710 | 43347 | 08$^h$ 49$^m$ 47.65$^s$ | −45° 18′ 28.5″ | 4.94 | −2.08 | 827 | A2III | |
| HD 72127 | | | 72127 | 41639 | 08$^h$ 29$^m$ 27.49$^s$ | −44° 43′ 29.4″ | 4.99 | −4.53 | 2610 | B2IV | suspected variable |
| GX Vel | | GX | 79186 | 45085 | 09$^h$ 11$^m$ 04.40$^s$ | −44° 52′ 04.5″ | 5.00 | −5.81 | 4700 | B5Ia | α Cyg variable, V$_{max}$ = 4.97$^m$, V$_{min}$ = 5.04$^m$ |
| HD 73155 | C | | 73155 | 42088 | 08$^h$ 34$^m$ 43.61$^s$ | −49° 56′ 39.3″ | 5.01 | −2.14 | 876 | K1/K2II | variable star, ΔV = 0.004$^m$, P = 0.091 d |
| HD 83058 | L | | 83058 | 46950 | 09$^h$ 34$^m$ 08.80$^s$ | −51° 15′ 19.0″ | 5.01 | −2.27 | 931 | B1.5IV | |
| HD 91504 | t | | 91504 | 51635 | 10$^h$ 32$^m$ 56.88$^s$ | −47° 00′ 12.1″ | 5.02 | −2.34 | 964 | K4III | |
| HD 67582 | | | 67582 | 39690 | 08$^h$ 06$^m$ 40.34$^s$ | −45° 15′ 57.8″ | 5.04 | −2.86 | 1240 | K3III | suspected variable, ΔV = 0.07$^m$ |
| HD 87783 | | | 87783 | 49485 | 10$^h$ 06$^m$ 11.22$^s$ | −47° 22′ 11.5″ | 5.06 | 0.57 | 258 | K0IV | |
| GU Vel | F | GU | 71935 | 41483 | 08$^h$ 27$^m$ 36.65$^s$ | −53° 05′ 18.7″ | 5.08 | 1.10 | 204 | A9/F0III/IV | δ Sct variable, V$_{max}$ = 5.08$^m$, V$_{min}$ = 5.11$^m$, P = 0.07 d |
| KX Vel | f | KX | 75821 | 43413 | 08$^h$ 50$^m$ 33.46$^s$ | −46° 31′ 45.1″ | 5.09 | −4.50 | 2694 | B0III | spectroscopic binary; Algol variable |
| HD 81848 | I | | 81848 | 46283 | 09$^h$ 26$^m$ 17.98$^s$ | −53° 22′ 44.2″ | 5.09 | −0.47 | 422 | B6V | variable star, ΔV = 0.008$^m$, P = 0.41 d |
| HD 85355 | u | | 85355 | 48224 | 09$^h$ 49$^m$ 57.16$^s$ | −45° 43′ 57.9″ | 5.09 | −2.01 | 856 | B7III | |
| ψ Vel B | ψ | | 82434B | | 09$^h$ 30$^m$ 42.11$^s$ | −40° 28′ 00.8″ | 5.12 | 3.75 | 61 | | suspected variable |
| HD 80108 | | | 80108 | 45505 | 09$^h$ 16$^m$ 23.04$^s$ | −44° 15′ 56.7″ | 5.12 | −5.34 | 4025 | K3Ib | variable star, ΔV = 0.006$^m$, P = 0.089 d |
| HD 82984 | | | 82984 | 46914 | 09$^h$ 33$^m$ 44.56$^s$ | −49° 00′ 18.3″ | 5.12 | −2.22 | 959 | B4IV | suspected variable |
| NO Vel | | NO | 69144 | 40285 | 08$^h$ 13$^m$ 36.16$^s$ | −46° 59′ 30.0″ | 5.14 | −2.23 | 970 | B2.5IV | eclipsing binary |
| HD 93563 | | | 93563 | 52742 | 10$^h$ 46$^m$ 57.49$^s$ | −56° 45′ 25.9″ | 5.14 | −0.99 | 548 | B8/B9III | variable star, ΔV = 0.003$^m$, P = 0.87 d |
| HD 74753 | D | | 74753 | 42834 | 08$^h$ 43$^m$ 40.28$^s$ | −49° 49′ 22.1″ | 5.15 | −3.19 | 1516 | B0IIIn | |
| FZ Vel | | FZ | 77140 | 44093 | 08$^h$ 58$^m$ 52.43$^s$ | −47° 14′ 05.4″ | 5.17 | 1.02 | 221 | Am | δ Sct variable, V$_{max}$ = 5.14$^m$, V$_{min}$ = 5.17$^m$, P = 0.065 d |
| HD 71510 | | | 71510 | 41296 | 08$^h$ 25$^m$ 31.34$^s$ | −51° 43′ 38.8″ | 5.18 | −1.40 | 674 | B2V | |
| NZ Vel | | NZ | 74146 | 42504 | 08$^h$ 39$^m$ 57.62$^s$ | −53° 03′ 17.2″ | 5.18 | −0.41 | 428 | B4IV | in IC 2391; rotating ellipsoidal variable |
| HD 68217 | | | 68217 | 39961 | 08$^h$ 09$^m$ 35.92$^s$ | −44° 07′ 22.0″ | 5.20 | −2.51 | 1136 | B2IV-V | suspected variable |
| NY Vel | | NY | 74067 | 42540 | 08$^h$ 40$^m$ 19.22$^s$ | −40° 15′ 50.0″ | 5.20 | 0.53 | 280 | Ap (SiCr) | α² CVn variable |
| LN Vel | | LN | 74371 | 42679 | 08$^h$ 41$^m$ 56.91$^s$ | −45° 24′ 38.6″ | 5.20 | −4.39 | 2694 | B5Iab | α Cyg variable, V$_{max}$ = 5.19$^m$, V$_{min}$ = 5.25$^m$, P = 8.29 d |
| IS Vel | | IS | 68324 | 39970 | 08$^h$ 09$^m$ 43.16$^s$ | −47° 56′ 14.0″ | 5.23 | −2.02 | 921 | B1IVe | β Cep variable |
| OY Vel | | OY | 77653 | 44337 | 09$^h$ 01$^m$ 44.57$^s$ | −52° 11′ 19.4″ | 5.23 | −0.41 | 437 | Ap Si | α² CVn variable |
| HD 79735 | z | | 79735 | 45344 | 09$^h$ 14$^m$ 24.50$^s$ | −43° 13′ 39.1″ | 5.24 | −0.92 | 556 | B4V+... | variable star, ΔV = 0.006$^m$, P = 0.71 d |
| HD 79846 | | | 79846 | 45328 | 09$^h$ 14$^m$ 18.02$^s$ | −55° 34′ 10.9″ | 5.26 | −1.20 | 638 | G8II/III | suspected variable |
| HD 80456 | K | | 80456 | 45631 | 09$^h$ 18$^m$ 05.89$^s$ | −51° 03′ 03.2″ | 5.26 | −0.34 | 431 | B7/B8III | |
| LW Vel | | LW | 88824 | 50070 | 10$^h$ 13$^m$ 22.88$^s$ | −51° 13′ 58.6″ | 5.27 | 1.78 | 163 | A7V | δ Sct variable, V$_{max}$ = 5.24$^m$, V$_{min}$ = 5.29$^m$, P = 0.11 d |
| HD 76360 | | | 76360 | 43671 | 08$^h$ 53$^m$ 50.60$^s$ | −47° 31′ 14.6″ | 5.31 | 0.79 | 261 | Am | |
| HD 80170 | | | 80170 | 45544 | 09$^h$ 16$^m$ 57.10$^s$ | −39° 24′ 05.2″ | 5.31 | 0.12 | 355 | K2III | |
| HD 72108 | A | | 72108 | 41616 | 08$^h$ 29$^m$ 04.76$^s$ | −47° 55′ 44.2″ | 5.33 | −3.18 | 1638 | B2IV | |
| HD 82694 | | | 82694 | 46811 | 09$^h$ 32$^m$ 19.27$^s$ | −40° 38′ 57.6″ | 5.35 | −0.04 | 390 | G8III | |
| OP Vel | | OP | 75149 | 43082 | 08$^h$ 46$^m$ 30.55$^s$ | −45° 54′ 45.1″ | 5.43 | −4.59 | 3293 | B3Ia | α Cyg variable |
| HD 83520 | | | 83520 | 47204 | 09$^h$ 37$^m$ 12.68$^s$ | −53° 40′ 06.5″ | 5.44 | 1.16 | 234 | A2/A3V | |
| HD 82419 | | | 82419 | 46594 | 09$^h$ 30$^m$ 05.13$^s$ | −51° 31′ 01.9″ | 5.45 | −0.08 | 415 | B8V | |
| HR 3440 | | HW | 74071 | 42459 | 08$^h$ 39$^m$ 23.87$^s$ | −53° 26′ 23.4″ | 5.46 | −0.24 | 451 | B5V | in IC 2391; β Cep variable, V$_{max}$ = 5.46$^m$, V$_{min}$ = 5.52$^m$, P = 0.26 d |
| HD 75630 | h | | 75630 | 43325 | 08$^h$ 49$^m$ 39.17$^s$ | −40° 19′ 12.6″ | 5.47 | −2.97 | 1590 | A2/A3IV | |
| HX Vel | | HX | 74455 | 42712 | 08$^h$ 42$^m$ 16.20$^s$ | −48° 05′ 56.8″ | 5.48 | −3.09 | 1689 | B1.5Vn | rotating ellipsoidal variable, V$_{max}$ = 5.48$^m$, V$_{min}$ = 5.53$^m$, P = 1.12 d |
| KT Vel | | KT | 74535 | 42715 | 08$^h$ 42$^m$ 19.02$^s$ | −53° 06′ 00.4″ | 5.49 | −0.36 | 483 | B8... | in IC 2391; α² CVn variable, V$_{max}$ = 5.49$^m$, V$_{min}$ = 5.56$^m$, P = 3.38 d |
| HD 83548 | y | | 83548 | 47267 | 09$^h$ 38$^m$ 01.43$^s$ | −43° 11′ 27.1″ | 5.51 | −0.35 | 484 | G8II | |
| HD 69194 | | | 69194 | 40282 | 08$^h$ 13$^m$ 34.23$^s$ | −50° 11′ 45.8″ | 5.51 | −1.29 | 753 | M1III | semiregular variable, ΔV = 0.07$^m$ |
| HD 74196 | | | 74196 | 42535 | 08$^h$ 40$^m$ 17.49$^s$ | −53° 00′ 55.6″ | 5.56 | −0.24 | 472 | B7Vn | in IC 2391; suspected β Cep variable, V$_{max}$ = 5.56$^m$, V$_{min}$ = 5.62$^m$ |
| HR 3600 | | IZ | 77475 | 44299 | 09$^h$ 01$^m$ 20.88$^s$ | −41° 51′ 51.4″ | 5.56 | −0.24 | 471 | B5V | slowly pulsating B star, V$_{max}$ = 5.53$^m$, V$_{min}$ = 5.56$^m$ |
| KL Vel | | KL | 79416 | 45189 | 09$^h$ 12$^m$ 30.54$^s$ | −43° 36′ 47.9″ | 5.56 | −0.85 | 623 | B8V | slowly pulsating B star, V$_{max}$ = 5.56$^m$, V$_{min}$ = 5.57$^m$, P = 2.91 d |
| HD 81034 | | | 81034 | 45924 | 09$^h$ 21$^m$ 50.94$^s$ | −42° 11′ 41.1″ | 5.56 | −0.63 | 565 | M3Ib | semiregular variable |
| HD 84461 | O | | 84461 | 47717 | 09$^h$ 43$^m$ 42.30$^s$ | −53° 53′ 28.9″ | 5.56 | 0.38 | 355 | A0V | |
| HD 84816 | | | 84816 | 47963 | 09$^h$ 46$^m$ 30.38$^s$ | −44° 45′ 18.2″ | 5.58 | −2.64 | 1436 | B2.5IV | suspected variable |
| HD 90677 | | | 90677 | 51140 | 10$^h$ 26$^m$ 48.93$^s$ | −54° 52′ 38.3″ | 5.58 | −2.87 | 1598 | K3II/III | variable star, ΔV = 0.008$^m$, P = 2.95 d |
| HD 89062 | | | 89062 | 50241 | 10$^h$ 15$^m$ 31.55$^s$ | −43° 06′ 44.1″ | 5.59 | −0.52 | 544 | K4III | |
| HD 81157 | | | 81157 | 45920 | 09$^h$ 21$^m$ 50.11$^s$ | −55° 30′ 53.5″ | 5.61 | 0.98 | 275 | A3IVs... | variable star, ΔV = 0.005$^m$, P = 0.090 d |
| HD 85563 | | | 85563 | 48348 | 09$^h$ 51$^m$ 19.76$^s$ | −46° 11′ 38.2″ | 5.62 | 0.56 | 335 | K2III | |
| NN Vel | | NN | 68161 | 39919 | 08$^h$ 09$^m$ 09.51$^s$ | −48° 41′ 03.9″ | 5.66 | −1.47 | 869 | B8Ib/II | α Cyg variable |
| HD 89736 | | | 89736 | 50609 | 10$^h$ 20$^m$ 16.72$^s$ | −47° 41′ 56.8″ | 5.66 | −3.93 | 2694 | K5/M0III | suspected variable |
| HD 74167 | | | 74167 | 42564 | 08$^h$ 40$^m$ 35.26$^s$ | −45° 11′ 28.0″ | 5.67 | −1.65 | 950 | M0III | variable star, ΔV = 0.013$^m$, P = 2.43 d |
| HD 96113 | | | 96113 | 54137 | 11$^h$ 04$^m$ 31.30$^s$ | −47° 40′ 45.1″ | 5.67 | 1.01 | 279 | A8III/IV | |
| HD 72737 | | | 72737 | 41861 | 08$^h$ 32$^m$ 04.97$^s$ | −53° 12′ 43.1″ | 5.68 | −1.56 | 913 | G8III+... | |
| HD 76653 | | | 76653 | 43797 | 08$^h$ 55$^m$ 11.76$^s$ | −54° 57′ 56.0″ | 5.70 | 3.79 | 79 | F6V | |
| HD 75276 | | | 75276 | 43148 | 08$^h$ 47$^m$ 18.85$^s$ | −46° 09′ 19.5″ | 5.71 | −4.52 | 3622 | F0Ib | |
| HD 86087 | | | 86087 | 48613 | 09$^h$ 54$^m$ 51.26$^s$ | −50° 14′ 38.3″ | 5.71 | 0.76 | 319 | A0V | |
| HD 85483 | | | 85483 | 48287 | 09$^h$ 50$^m$ 41.97$^s$ | −46° 56′ 02.4″ | 5.72 | −0.59 | 597 | K0IIICN... | suspected variable |
| HD 85980 | | | 85980 | 48561 | 09$^h$ 54$^m$ 17.67$^s$ | −45° 17′ 00.7″ | 5.72 | −1.35 | 845 | B+... | |
| HD 81136 | | | 81136 | 45962 | 09$^h$ 22$^m$ 24.00$^s$ | −46° 02′ 51.0″ | 5.74 | −0.47 | 570 | G6/G8III | suspected variable, V$_{max}$ = 5.72$^m$, V$_{min}$ = 5.77$^m$ |
| HD 91355 | s | | 91355 | 51561 | 10$^h$ 31$^m$ 57.45$^s$ | −45° 04′ 00.2″ | 5.76 | 0.00 | 463 | B9 | suspected variable, V$_{max}$ = 5.75$^m$, V$_{min}$ = 5.78$^m$ |
| AH Vel | | AH | 68808 | 40155 | 08$^h$ 11$^m$ 59.97$^s$ | −46° 38′ 39.7″ | 5.76 | −2.50 | 1462 | F7p | classical Cepheid, V$_{max}$ = 5.5$^m$, V$_{min}$ = 5.89$^m$, P = 4.23 d |
| HD 79275 | | | 79275 | 45122 | 09$^h$ 11$^m$ 33.39$^s$ | −46° 35′ 02.1″ | 5.78 | −1.95 | 1144 | B2IV-V | |
| HD 88842 | | | 88842 | 50078 | 10$^h$ 13$^m$ 28.04$^s$ | −51° 45′ 20.9″ | 5.78 | 0.83 | 318 | A3IV/V | |
| HR 3413 | E | HV | 73340 | 42177 | 08$^h$ 35$^m$ 52.04$^s$ | −50° 58′ 10.8″ | 5.79 | 0.01 | 466 | B8 Si | rapidly oscillating Ap star, V$_{max}$ = 5.77$^m$, V$_{min}$ = 5.81$^m$, P = 2.67 d |
| HD 76110 | | | 76110 | 43603 | 08$^h$ 52$^m$ 48.02$^s$ | −38° 43′ 26.9″ | 5.79 | −1.36 | 876 | K5/M0III | suspected variable |
| HD 89569 | | | 89569 | 50493 | 10$^h$ 18$^m$ 38.16$^s$ | −56° 06′ 38.4″ | 5.80 | 3.03 | 117 | F6V | suspected variable |
| HD 95347 | | | 95347 | 53762 | 10$^h$ 59$^m$ 59.43$^s$ | −43° 48′ 25.7″ | 5.81 | 1.07 | 290 | B8/B9V | |
| HD 72067 | | | 72067 | 41621 | 08$^h$ 29$^m$ 07.57$^s$ | −44° 09′ 37.6″ | 5.82 | −2.63 | 1598 | B2V | suspected variable, V$_{max}$ = 5.75$^m$, V$_{min}$ = 5.90$^m$ |
| HD 68657 | | | 68657 | 40077 | 08$^h$ 11$^m$ 10.80$^s$ | −48° 27′ 43.2″ | 5.83 | −0.91 | 728 | B3V | suspected variable |
| LR Vel | | LR | 80558 | 45675 | 09$^h$ 18$^m$ 42.36$^s$ | −51° 33′ 38.4″ | 5.83 | −4.77 | 4200 | B7Iab | α Cyg variable, V$_{max}$ = 5.82$^m$, V$_{min}$ = 5.96$^m$, P = 1.69 d |
| HD 79694 | | | 79694 | 45314 | 09$^h$ 14$^m$ 08.23$^s$ | −44° 08′ 45.1″ | 5.85 | −0.17 | 521 | B6IV | suspected variable, V$_{max}$ = 5.80$^m$, V$_{min}$ = 5.85$^m$ |
| HD 79807 | k$^1$ | | 79807 | 45386 | 09$^h$ 14$^m$ 57.17$^s$ | −37° 36′ 08.5″ | 5.85 | −0.57 | 627 | K0/K1III+.. | |
| HD 69302 | | | 69302 | 40357 | 08$^h$ 14$^m$ 23.88$^s$ | −45° 50′ 04.4″ | 5.86 | −1.35 | 903 | B2IV-V | |
| HD 77020 | | | 77020 | 44024 | 08$^h$ 57$^m$ 55.57$^s$ | −48° 34′ 22.6″ | 5.88 | −1.71 | 1072 | G8/K0II | |
| HD 71043 | | | 71043 | 41081 | 08$^h$ 22$^m$ 55.18$^s$ | −52° 07′ 25.6″ | 5.89 | 1.57 | 238 | A0V | |
| HD 74273 | | | 74273 | 42614 | 08$^h$ 41$^m$ 05.32$^s$ | −48° 55′ 21.7″ | 5.90 | −2.56 | 1606 | B1.5V | |
| IW Vel | | IW | 94985 | 53530 | 10$^h$ 57$^m$ 07.88$^s$ | −50° 45′ 54.2″ | 5.90 | 0.96 | 317 | A7Vni | δ Sct variable, ΔV = 0.016$^m$, P = 0.15 d |
| HD 91437 | | | 91437 | 51610 | 10$^h$ 32$^m$ 33.62$^s$ | −44° 37′ 06.4″ | 5.91 | 0.48 | 397 | G6/G8III | |
| HD 72832 | | | 72832 | 42001 | 08$^h$ 33$^m$ 38.45$^s$ | −38° 50′ 55.8″ | 5.92 | −1.10 | 825 | B5III | suspected variable |
| HD 76161 | | | 76161 | 43589 | 08$^h$ 52$^m$ 38.62$^s$ | −48° 21′ 32.8″ | 5.92 | −1.69 | 1087 | B3Vn | |
| HD 79621 | | | 79621 | 45270 | 09$^h$ 13$^m$ 34.48$^s$ | −47° 20′ 18.4″ | 5.92 | −0.23 | 554 | B9V | |
| V335 Vel | | V335 | 85953 | 48527 | 09$^h$ 53$^m$ 50.11$^s$ | −51° 08′ 48.2″ | 5.95 | −2.64 | 1707 | B2V | slowly pulsating B star, V$_{max}$ = 5.93$^m$, V$_{min}$ = 5.97$^m$, P = 3.76 d |
| HD 67249 | | | 67249 | 39527 | 08$^h$ 04$^m$ 42.41$^s$ | −50° 35′ 25.4″ | 5.96 | −2.14 | 1358 | G5II | |
| HD 89461 | | | 89461 | 50480 | 10$^h$ 18$^m$ 28.27$^s$ | −41° 40′ 06.6″ | 5.97 | −0.17 | 551 | B9V | |
| HD 72232 | | | 72232 | 41674 | 08$^h$ 29$^m$ 45.65$^s$ | −46° 19′ 54.2″ | 5.98 | −0.45 | 629 | B7IV | variable star, ΔV = 0.006$^m$, P = 0.83 d |
| HD 88399 | | | 88399 | 49844 | 10$^h$ 10$^m$ 37.70$^s$ | −41° 42′ 53.8″ | 5.98 | 1.81 | 223 | K3III | |
| HD 84228 | | | 84228 | 47559 | 09$^h$ 41$^m$ 47.94$^s$ | −55° 12′ 49.6″ | 5.99 | −3.60 | 2694 | B4V | suspected variable |
| HD 68895 | | | 68895 | 40183 | 08$^h$ 12$^m$ 30.80$^s$ | −46° 15′ 51.5″ | 6.00 | −0.68 | 706 | B5V | |
| HD 75759 | | | 75759 | 43392 | 08$^h$ 50$^m$ 21.02$^s$ | −42° 05′ 23.3″ | 6.00 | −2.84 | 1906 | O9V | |
| HD 80057 | | | 80057 | 45481 | 09$^h$ 16$^m$ 04.03$^s$ | −44° 53′ 55.4″ | 6.02 | −4.60 | 4347 | A1Ib+... | suspected variable, V$_{max}$ = 6.01$^m$, V$_{min}$ = 6.05$^m$ |
| IU Vel | | IU | 77320 | 44213 | 09$^h$ 00$^m$ 22.26$^s$ | −43° 10′ 26.4″ | 6.04 | −1.39 | 1000 | B3Vne | γ Cas variable, V$_{max}$ = 5.97$^m$, V$_{min}$ = 6.08$^m$ |
| HD 80774 | | | 80774 | 45814 | 09$^h$ 20$^m$ 29.68$^s$ | −37° 34′ 53.9″ | 6.04 | 0.05 | 513 | K3/K4III | |
| HD 91356 | | | 91356 | 51560 | 10$^h$ 31$^m$ 56.65$^s$ | −45° 04′ 10.8″ | 6.04 | 0.21 | 477 | B4 | |
| HD 71722 | | | 71722 | 41373 | 08$^h$ 26$^m$ 25.24$^s$ | −52° 48′ 27.0″ | 6.05 | 1.79 | 232 | A0V | |
| HD 79241 | | | 79241 | 45127 | 09$^h$ 11$^m$ 40.95$^s$ | −39° 15′ 31.9″ | 6.05 | −1.92 | 1278 | B5III | |
| HD 81471 | | | 81471 | 46093 | 09$^h$ 23$^m$ 59.34$^s$ | −51° 44′ 13.5″ | 6.05 | −5.17 | 5719 | A7Iab | suspected α Cyg variable |
| HD 81411 | | | 81411 | 46114 | 09$^h$ 24$^m$ 16.28$^s$ | −39° 25′ 31.6″ | 6.05 | 0.04 | 518 | A6/A7III | |
| HD 85250 | | | 85250 | 48119 | 09$^h$ 48$^m$ 40.06$^s$ | −56° 24′ 42.9″ | 6.05 | 1.01 | 332 | K0III | |
| HD 86523 | | | 86523 | 48835 | 09$^h$ 57$^m$ 42.61$^s$ | −48° 24′ 50.7″ | 6.06 | −4.27 | 3791 | B3V | |
| HD 91805 | | | 91805 | 51816 | 10$^h$ 35$^m$ 10.45$^s$ | −43° 39′ 52.8″ | 6.09 | −1.12 | 901 | G8/K0II/III | |
| HD 78548 | | | 78548 | 44708 | 09$^h$ 06$^m$ 34.04$^s$ | −55° 48′ 08.7″ | 6.10 | −1.70 | 1185 | B2IV-V | suspected variable |
| HD 90798 | | | 90798 | 51245 | 10$^h$ 28$^m$ 02.08$^s$ | −49° 24′ 20.5″ | 6.10 | −1.15 | 921 | K4III | suspected variable, V$_{max}$ = 6.08$^m$, V$_{min}$ = 6.12$^m$ |
| HD 92328 | | | 92328 | 52112 | 10$^h$ 38$^m$ 50.33$^s$ | −42° 45′ 12.3″ | 6.10 | −0.11 | 569 | Am+... | |
| KQ Vel | | KQ | 94660 | 53379 | 10$^h$ 55$^m$ 01.04$^s$ | −42° 15′ 03.9″ | 6.11 | 0.23 | 489 | A0sp... | α² CVn variable, V$_{max}$ = 6.1$^m$, V$_{min}$ = 6.12$^m$ |
| HD 87363 | | | 87363 | 49259 | 10$^h$ 03$^m$ 20.60$^s$ | −46° 38′ 10.2″ | 6.11 | 1.29 | 300 | A0V | |
| HD 96224 | | | 96224 | 54185 | 11$^h$ 05$^m$ 04.14$^s$ | −49° 23′ 32.4″ | 6.11 | 0.12 | 514 | B9V | |
| IV Vel | | IV | 86466 | 48799 | 09$^h$ 57$^m$ 10.95$^s$ | −52° 38′ 19.7″ | 6.13 | −3.98 | 3432 | B3IV | β Cep variable |
| HD 90518 | | | 90518 | 51077 | 10$^h$ 26$^m$ 09.91$^s$ | −42° 44′ 18.2″ | 6.13 | 1.09 | 332 | K1III | |
| IP Vel | | IP | 84400 | 47694 | 09$^h$ 43$^m$ 27.60$^s$ | −51° 13′ 41.4″ | 6.15 | −1.96 | 1364 | B6V | Algol variable |
| HD 95429 | | | 95429 | 53771 | 11$^h$ 00$^m$ 08.34$^s$ | −51° 49′ 04.1″ | 6.15 | 2.26 | 195 | A3III/IV | |
| HD 88693 | | | 88693 | 49994 | 10$^h$ 12$^m$ 22.97$^s$ | −52° 09′ 48.1″ | 6.16 | 1.11 | 334 | K2IIICN... | suspected variable |
| HD 89104 | | | 89104 | 50232 | 10$^h$ 15$^m$ 16.65$^s$ | −54° 58′ 27.2″ | 6.16 | −2.04 | 1424 | B2IV-V | suspected variable |
| MX Vel | | MX | 67341 | 39584 | 08$^h$ 05$^m$ 20.31$^s$ | −46° 58′ 42.3″ | 6.18 | −2.68 | 1929 | B3Vnp | Be star |
| HR 3831 | | IM | 83368 | 47145 | 09$^h$ 36$^m$ 25.41$^s$ | −48° 45′ 04.2″ | 6.18 | 1.88 | 236 | F0p | rapidly oscillating Ap star |
| HD 83465 | | | 83465 | 47172 | 09$^h$ 36$^m$ 46.41$^s$ | −52° 56′ 38.1″ | 6.18 | 0.80 | 388 | K1III | |
| HD 90393 | | | 90393 | 51014 | 10$^h$ 25$^m$ 17.22$^s$ | −42° 28′ 02.5″ | 6.18 | −0.09 | 586 | G8III | |
| HD 79091 | | | 79091 | 45002 | 09$^h$ 09$^m$ 57.15$^s$ | −52° 04′ 58.8″ | 6.19 | 1.34 | 304 | K1III | |
| HD 81780 | | | 81780 | 46297 | 09$^h$ 26$^m$ 28.45$^s$ | −40° 30′ 06.2″ | 6.19 | 1.37 | 300 | A7III | |
| HD 87152 | | | 87152 | 49137 | 10$^h$ 01$^m$ 40.73$^s$ | −53° 21′ 50.8″ | 6.20 | −2.03 | 1442 | B2.5V | variable star, V$_{max}$ = 6.18$^m$, V$_{min}$ = 6.20$^m$, P = 3.79 d |
| HD 75081 | | | 75081 | 43073 | 08$^h$ 46$^m$ 23.77$^s$ | −41° 07′ 31.4″ | 6.21 | −0.51 | 720 | B9V | |
| HD 81369 | | | 81369 | 46067 | 09$^h$ 23$^m$ 39.77$^s$ | −46° 54′ 31.6″ | 6.21 | −1.49 | 1128 | B7III | |
| HD 87652 | | | 87652 | 49394 | 10$^h$ 05$^m$ 01.86$^s$ | −51° 18′ 49.1″ | 6.23 | 0.17 | 532 | B8/B9III | |
| HD 90170 | | | 90170 | 50903 | 10$^h$ 23$^m$ 40.71$^s$ | −41° 57′ 11.6″ | 6.24 | 1.98 | 232 | K0IV | |
| HD 72900 | | | 72900 | 41986 | 08$^h$ 33$^m$ 30.28$^s$ | −46° 58′ 14.4″ | 6.25 | −2.66 | 1976 | K3III | |
| HD 77580 | | | 77580 | 44367 | 09$^h$ 02$^m$ 06.42$^s$ | −39° 24′ 08.1″ | 6.25 | 1.05 | 357 | K1IIICN... | |
| HD 79900 | | | 79900 | 45413 | 09$^h$ 15$^m$ 14.64$^s$ | −45° 33′ 19.8″ | 6.25 | −2.47 | 1811 | B8V | |
| HR 3562 | | IY | 76566 | 43807 | 08$^h$ 55$^m$ 19.21$^s$ | −45° 02′ 30.1″ | 6.26 | −1.03 | 934 | B3IV | slowly pulsating B star, V$_{max}$ = 6.23$^m$, V$_{min}$ = 6.27$^m$ |
| HD 79524 | | | 79524 | 45242 | 09$^h$ 13$^m$ 18.68$^s$ | −42° 16′ 24.4″ | 6.27 | 0.48 | 469 | K2III | |
| HD 81347 | | | 81347 | 46045 | 09$^h$ 23$^m$ 25.38$^s$ | −48° 17′ 13.0″ | 6.27 | −1.88 | 1393 | B5V | suspected variable, V$_{max}$ = 6.25$^m$, V$_{min}$ = 6.29$^m$ |
| HD 80781 | | | 80781 | 45742 | 09$^h$ 19$^m$ 32.49$^s$ | −55° 11′ 11.4″ | 6.28 | −3.83 | 3432 | B5V | |
| HD 75466 | | | 75466 | 43195 | 08$^h$ 48$^m$ 00.24$^s$ | −52° 51′ 00.7″ | 6.29 | 0.52 | 464 | B8V | |
| HD 93453 | | | 93453 | 52709 | 10$^h$ 46$^m$ 37.14$^s$ | −43° 11′ 33.1″ | 6.29 | 1.91 | 245 | A4IV | |
| HD 72993 | | | 72993 | 42070 | 08$^h$ 34$^m$ 29.26$^s$ | −37° 36′ 40.3″ | 6.30 | −1.11 | 988 | M0III | suspected variable, ΔV = 0.09$^m$ |
| GY Vel | | GY | 89273 | 50332 | 10$^h$ 16$^m$ 40.17$^s$ | −51° 12′ 16.8″ | 6.30 | −0.41 | 715 | M4/M5III | semiregular variable, V$_{max}$ = 6.23$^m$, V$_{min}$ = 6.5$^m$ |
| HD 72350 | | | 72350 | 41737 | 08$^h$ 30$^m$ 39.24$^s$ | −44° 44′ 14.4″ | 6.30 | −2.88 | 2233 | B4V | |
| HD 79523 | | | 79523 | 45259 | 09$^h$ 13$^m$ 25.82$^s$ | −38° 36′ 59.2″ | 6.31 | −0.40 | 715 | A0V | |
| GK Vel | | GK | 81575 | 46194 | 09$^h$ 25$^m$ 07.89$^s$ | −43° 58′ 36.1″ | 6.31 | −0.61 | 789 | M5III | semiregular variable, V$_{max}$ = 6.26$^m$, V$_{min}$ = 6.39$^m$, P = 120 d |
| HD 80435 | | | 80435 | 45603 | 09$^h$ 17$^m$ 42.31$^s$ | −54° 29′ 41.5″ | 6.33 | −0.65 | 811 | K3III | |
| HD 67621 | | | 67621 | 39691 | 08$^h$ 06$^m$ 41.61$^s$ | −48° 29′ 50.7″ | 6.34 | −1.78 | 1370 | B3III | |
| HD 72650 | | | 72650 | 41813 | 08$^h$ 31$^m$ 29.57$^s$ | −54° 23′ 38.1″ | 6.34 | 0.45 | 491 | K3III | |
| HD 75289 | | | 75289 | 43177 | 08$^h$ 47$^m$ 40.41$^s$ | −41° 44′ 10.5″ | 6.35 | 4.04 | 94 | G0V | has a planet (b) |
| HD 72798 | | | 72798 | 41941 | 08$^h$ 33$^m$ 01.87$^s$ | −45° 45′ 10.5″ | 6.36 | −3.02 | 2451 | B5III | |
| HD 76004 | | | 76004 | 43520 | 08$^h$ 51$^m$ 50.05$^s$ | −44° 09′ 03.4″ | 6.38 | −1.60 | 1283 | B3V | |
| HZ Vel | | HZ | 75654 | 43354 | 08$^h$ 49$^m$ 52.40$^s$ | −39° 08′ 30.1″ | 6.39 | 1.93 | 254 | A5III | δ Sct variable, ΔV = 0.025$^m$, P = 0.087 d |
| HD 72485 | | | 72485 | 41781 | 08$^h$ 31$^m$ 10.64$^s$ | −47° 51′ 59.9″ | 6.39 | −1.15 | 1052 | B2.5V | |
| HD 76230 | | | 76230 | 43593 | 08$^h$ 52$^m$ 40.83$^s$ | −52° 07′ 44.2″ | 6.39 | 0.67 | 453 | A0V | |
| HD 77907 | | | 77907 | 44423 | 09$^h$ 03$^m$ 05.35$^s$ | −53° 33′ 01.4″ | 6.39 | −0.72 | 862 | B6V | |
| HD 86211 | | | 86211 | 48706 | 09$^h$ 56$^m$ 05.35$^s$ | −40° 49′ 28.2″ | 6.39 | −0.67 | 840 | M1III | suspected variable |
| HD 86352 | | | 86352 | 48730 | 09$^h$ 56$^m$ 21.90$^s$ | −51° 20′ 10.2″ | 6.39 | −4.38 | 4657 | B2IV-V | |
| HD 88015 | | | 88015 | 49619 | 10$^h$ 07$^m$ 35.73$^s$ | −48° 15′ 39.0″ | 6.40 | −1.60 | 1299 | B3III | |
| HD 94724 | | | 94724 | 53411 | 10$^h$ 55$^m$ 27.25$^s$ | −43° 01′ 14.0″ | 6.40 | 1.44 | 320 | A0V | |
| HD 76304 | | | 76304 | 43673 | 08$^h$ 53$^m$ 50.76$^s$ | −40° 26′ 51.2″ | 6.42 | −1.61 | 1315 | K0II/III+.. | |
| HD 87122 | | | 87122 | 49092 | 10$^h$ 01$^m$ 12.01$^s$ | −56° 05′ 47.6″ | 6.42 | −0.70 | 867 | B8 | |
| HD 75387 | | | 75387 | 43209 | 08$^h$ 48$^m$ 08.79$^s$ | −42° 27′ 48.5″ | 6.43 | −2.15 | 1698 | B2IV | suspected variable |
| HD 92155 | | | 92155 | 51984 | 10$^h$ 37$^m$ 16.12$^s$ | −53° 51′ 19.0″ | 6.43 | −2.10 | 1655 | B3Vn | |
| HD 69596 | | | 69596 | 40433 | 08$^h$ 15$^m$ 23.27$^s$ | −50° 26′ 57.1″ | 6.44 | −0.32 | 734 | K3/K4III | |
| HD 73121 | | | 73121 | 42123 | 08$^h$ 35$^m$ 12.48$^s$ | −39° 58′ 14.0″ | 6.44 | 3.64 | 118 | G1V | |
| HD 95509 | | | 95509 | 53811 | 11$^h$ 00$^m$ 36.33$^s$ | −53° 06′ 42.7″ | 6.44 | 0.92 | 415 | K3III | |
| HD 69404 | | | 69404 | 40397 | 08$^h$ 14$^m$ 51.25$^s$ | −46° 29′ 09.3″ | 6.45 | −1.60 | 1331 | B3Vnne | γ Cas variable, V$_{max}$ = 6.37$^m$, V$_{min}$ = 6.46$^m$ |
| HD 70309 | | | 70309 | 40749 | 08$^h$ 19$^m$ 05.60$^s$ | −48° 11′ 52.4″ | 6.45 | −0.56 | 823 | B3V | |
| HD 73952 | | | 73952 | 42400 | 08$^h$ 38$^m$ 44.83$^s$ | −53° 05′ 25.6″ | 6.45 | 0.50 | 505 | B8Vn | in IC 2391 |
| HD 94508 | | | 94508 | 53260 | 10$^h$ 53$^m$ 33.42$^s$ | −56° 25′ 13.8″ | 6.45 | | 4100 | K2III | |
| HD 68478 | | | 68478 | 40016 | 08$^h$ 10$^m$ 20.57$^s$ | −49° 14′ 14.5″ | 6.46 | −2.03 | 1630 | B3IV | |
| HD 78005 | | | 78005 | 44509 | 09$^h$ 04$^m$ 05.79$^s$ | −47° 26′ 29.3″ | 6.46 | −1.27 | 1144 | B4V | suspected variable |
| HD 81309 | | | 81309 | 46075 | 09$^h$ 23$^m$ 44.92$^s$ | −37° 45′ 25.1″ | 6.47 | 1.45 | 329 | A1m... | |
| QZ Vel | | QZ | 85871 | 48469 | 09$^h$ 53$^m$ 00.11$^s$ | −55° 22′ 23.6″ | 6.48 | −3.06 | 2650 | B1IIIn | slowly pulsating B star |
| HD 68763 | | | 68763 | 40160 | 08$^h$ 12$^m$ 06.06$^s$ | −43° 24′ 01.6″ | 6.48 | −5.11 | 6792 | K3III: | suspected variable |
| HD 72787 | | | 72787 | 41970 | 08$^h$ 33$^m$ 19.87$^s$ | −38° 22′ 14.5″ | 6.48 | −1.63 | 1364 | B2/B3V | suspected variable |
| HD 79025 | | | 79025 | 44979 | 09$^h$ 09$^m$ 45.00$^s$ | −49° 25′ 27.5″ | 6.48 | 0.49 | 513 | A9Vn | |
| HD 88862 | | | 88862 | 50069 | 10$^h$ 13$^m$ 22.32$^s$ | −56° 35′ 12.1″ | 6.48 | −0.53 | 821 | K2III | |
| HD 89328 | | | 89328 | 50391 | 10$^h$ 17$^m$ 20.20$^s$ | −46° 50′ 05.8″ | 6.48 | 2.51 | 203 | A8V+... | |
| V361 Vel | | V361 | 95716 | 53940 | 11$^h$ 02$^m$ 13.84$^s$ | −41° 06′ 50.6″ | 6.48 | −2.18 | 1762 | M4III | semiregular variable, V$_{max}$ = 6.17$^m$, V$_{min}$ = 6.88$^m$, P = 64.9 d |
| HD 69168 | | | 69168 | 40299 | 08$^h$ 13$^m$ 45.66$^s$ | −46° 34′ 43.3″ | 6.49 | −0.96 | 1009 | B3V | |
| HD 71805 | | | 71805 | 41426 | 08$^h$ 26$^m$ 57.83$^s$ | −52° 42′ 17.4″ | 6.49 | 2.82 | 176 | F5V... | |
| HD 72752 | | | 72752 | 41905 | 08$^h$ 32$^m$ 40.51$^s$ | −47° 02′ 31.7″ | 6.49 | −0.01 | 651 | K2III | |
| HD 75989 | | | 75989 | 43528 | 08$^h$ 51$^m$ 55.60$^s$ | −40° 59′ 11.8″ | 6.49 | −1.18 | 1113 | Ap... | |
| HD 87030 | | | 87030 | 49052 | 10$^h$ 00$^m$ 34.58$^s$ | −56° 56′ 46.2″ | 6.50 | 0.52 | 511 | K0III | |
| R Vel | | R | 87816 | 49477 | 10$^h$ 06$^m$ 07.26$^s$ | −52° 11′ 16.7″ | 6.51 | 1.09 | 394 | K0III | suspected variable, V$_{max}$ = 6.49$^m$, V$_{min}$ = 6.52$^m$ |
| HD 72436 | | | 72436 | 41806 | 08$^h$ 31$^m$ 24.70$^s$ | −39° 03′ 50.9″ | 6.52 | −1.80 | 1500 | B5V | suspected variable |
| CV Vel | | CV | 77464 | 44245 | 09$^h$ 00$^m$ 37.99$^s$ | −51° 33′ 20.1″ | 6.69 | | 1430 | B2V+... | Algol variable, V$_{max}$ = 6.69$^m$, V$_{min}$ = 7.19$^m$, P = 6.89 d |
| AI Vel | | AI | 69213 | 40330 | 08$^h$ 14$^m$ 05.15$^s$ | −44° 34′ 32.8″ | 6.70 | | 319 | A9IV/V | double-mode δ Sct variable, V$_{max}$ = 6.15$^m$, V$_{min}$ = 6.76$^m$, P = 0.11 d |
| KK Vel | | KK | 78616 | 44790 | 09$^h$ 07$^m$ 42.52$^s$ | −44° 37′ 56.8″ | 6.79 | | 1650 | B2II/III | β Cep variable |
| Vela X-1 | | GP | 77581 | 44368 | 09$^h$ 02$^m$ 06.86$^s$ | −40° 33′ 16.9″ | 6.87 | | 3500 | B0.5Iae | X-ray pulsar system and eclipsing binary, V$_{max}$ = 6.76$^m$, V$_{min}$ = 6.99$^m$, P = 8.96 d |
| HD 72754 | | FY | 72754 | 41882 | 08$^h$ 32$^m$ 23.38$^s$ | −49° 36′ 04.8″ | 6.90 | | 2160 | B2Ia:pshe | β Lyr variable, V$_{max}$ = 6.84$^m$, V$_{min}$ = 7.06$^m$, P = 33.72 d |
| RZ Vel | | RZ | 73502 | 42257 | 08$^h$ 37$^m$ 01.30$^s$ | −44° 06′ 52.8″ | 7.13 | | 1770 | G1Ib | classical Cepheid, V$_{max}$ = 6.42$^m$, V$_{min}$ = 7.64$^m$, P = 20.40 d |
| HD 73882 | | NX | 73882 | 42433 | 08$^h$ 39$^m$ 09.53$^s$ | −40° 25′ 09.3″ | 7.19 | | 1500 | O9III | Algol variable, V$_{max}$ = 7.19$^m$, V$_{min}$ = 7.29$^m$, P = 2.92 d |
| V342 Vel | | V342 | 89767 | 50598 | 10$^h$ 20$^m$ 11.74$^s$ | −52° 36′ 06.2″ | 7.23 | −6.4 | 6000 | B0Iab | α Cyg variable, V$_{max}$ = 7.16$^m$, V$_{min}$ = 7.25$^m$ |
| HD 93385 | | | 93385 | 52676 | 10$^h$ 46$^m$ 15$^s$ | −41° 27′ 52″ | 7.49 | | 138 | G2V | has two planets (b & c) |
| HD 76534 | | OU | 76534 | 43792 | 08$^h$ 55$^m$ 08.71$^s$ | −43° 27′ 59.9″ | 7.50 | | 3200 | B2Vne | Be star |
| IGR J08408-4503 | | LM | 74194 | 42587 | 08$^h$ 40$^m$ 47.79$^s$ | −45° 03′ 30.2″ | 7.55 | | | O8Ib(f) | recurrent X-ray transient and α Cyg variable, V$_{max}$ = 7.54$^m$, V$_{min}$ = 7.57$^m$, P = 7.81 d |
| HD 74438 | | | | | 08$^h$ 38$^m$ 9$^s$ | −52° 42′ 0″ | 7.58 | | 500 | A3 | Quadruple star, consists of two binary stars, orbiting their barycenter. |
| HD 85512 | | | 85512 | 48331 | 09$^h$ 51$^m$ 07$^s$ | −43° 30′ 10″ | 7.67 | | 36 | K5V | has a planet (b) |
| HD 80077 | | PV | 80077 | 45467 | 09$^h$ 15$^m$ 54.79$^s$ | −49° 58′ 24.6″ | 7.68 | | | B2Ia+e | possibly in Pismis 11; luminous blue variable, V$_{max}$ = 7.42$^m$, V$_{min}$ = 7.68$^m$ |
| T Vel | | T | 73678 | 42321 | 08$^h$ 37$^m$ 40.83$^s$ | −47° 21′ 43.1″ | 7.68 | | 7100 | G0II | classical Cepheid, V$_{max}$ = 7.68$^m$, V$_{min}$ = 8.34$^m$, P = 4.64 d |
| S Vel | | S | 82829 | 46881 | 09$^h$ 33$^m$ 13.20$^s$ | −45° 12′ 30.9″ | 7.81 | | 512 | A5m | Algol variable, V$_{max}$ = 7.74$^m$, V$_{min}$ = 9.5$^m$, P = 5.93 d |
| SV Vel | | SV | 93247 | 52570 | 10$^h$ 44$^m$ 56.35$^s$ | −56° 17′ 22.4″ | 7.91 | | | F7II | classical Cepheid, V$_{max}$ = 7.91$^m$, V$_{min}$ = 9.12$^m$, P = 14.10 d |
| AX Vel | | AX | 68556 | | 08$^h$ 10$^m$ 49.32$^s$ | −47° 41′ 54.8″ | 8.16 | | | F6II | double-mode Cepheid variable, V$_{max}$ = 7.93$^m$, V$_{min}$ = 8.48$^m$, P = 2.59 d |
| HD 83443 | | | 83443 | 47202 | 09$^h$ 37$^m$ 11.83$^s$ | −43° 16′ 19.9″ | 8.24 | 5.05 | 142 | K0V | Kalausi, has a planet (b) |
| W Vel | | W | 299011 | 50230 | 10$^h$ 15$^m$ 14.83$^s$ | −54° 28′ 42.0″ | 8.30 | | 967 | M8IIIe | Mira variable, V$_{max}$ = 8.2$^m$, V$_{min}$ = 14.4$^m$, P = 395 d |
| SW Vel | | SW | 74712 | 42831 | 08$^h$ 43$^m$ 38.69$^s$ | −47° 24′ 11.2″ | 8.32 | | 5300 | F9Ib | classical Cepheid, V$_{max}$ = 7.49$^m$, V$_{min}$ = 8.75$^m$, P = 23.41 d |
| SX Vel | | SX | 74884 | 42926 | 08$^h$ 44$^m$ 53.47$^s$ | −46° 20′ 34.8″ | 8.33 | | 3050 | F8II | classical Cepheid, V$_{max}$ = 7.92$^m$, V$_{min}$ = 8.72$^m$, P = 9.55 d |
| HD 85390 | | | 85390 | 48235 | 09$^h$ 50$^m$ 02.0$^s$ | −49° 47′ 25″ | 8.54 | 5.90 | 111 | K1V | Natasha, has two planets (b & c) |
| HD 95338 | | | 95338 | 53719 | 10$^h$ 59$^m$ 26.3$^s$ | −45° 39′ 33.1″ | 8.62 | 5.72 | 120.79 | K0.5V | has a transiting planet (b) |
| AL Vel | | AL | | 41784 | 08$^h$ 31$^m$ 11.28$^s$ | −47° 39′ 57.4″ | 8.65 | | | K0III+A3III/V | Algol variable, V$_{max}$ = 8.6$^m$, V$_{min}$ = 8.93$^m$, P = 96.11 d |
| WY Vel | | WY | 81137 | | 09$^h$ 21$^m$ 59.19$^s$ | −52° 33′ 51.8″ | 8.80 | | | M2pe | Z And variable, V$_{max}$ = 7.50$^m$, V$_{min}$ = 9.1$^m$ |
| HD 73526 | | | 73526 | 42282 | 08$^h$ 37$^m$ 16.48$^s$ | −41° 19′ 08.8″ | 9.00 | 4.12 | 309 | G6V | has two planets (b & c) |
| IRAS 08544-4431 | | V390 | | | 08$^h$ 56$^m$ 14.19$^s$ | −44° 43′ 10.8″ | 9.18 | | 2600 | F3e | post-AGB star; semiregular variable, V$_{max}$ = 9.01$^m$, V$_{min}$ = 9.27$^m$, P = 94.73 d |
| AO Vel | | AO | 68826 | | 08$^h$ 11$^m$ 53.91$^s$ | −48° 44′ 46.0″ | 9.37 | | | B9III | trinary star; Algol variable V$_{max}$ = 9.35$^m$, V$_{min}$ = 9.79$^m$, P = 1.58 d |
| AP Vel | | AP | | 42492 | 08$^h$ 39$^m$ 45.76$^s$ | −43° 51′ 39.2″ | 10.16 | | 4600 | F9 | double-mode Cepheid variable, V$_{max}$ = 9.49$^m$, V$_{min}$ = 10.48$^m$, P = 3.13 d |
| AF Vel | | AF | | 53213 | 10$^h$ 53$^m$ 02.49$^s$ | −49° 54′ 22.7″ | 10.69 | | 2250 | F2.5 | RR Lyr variable, V$_{max}$ = 10.68$^m$, V$_{min}$ = 11.78$^m$, P = 0.53 d |
| WR 12 | | V378 | | | 08$^h$ 44$^m$ 47.29$^s$ | −45° 58′ 55.5″ | 10.78 | | | WN8h+? | Algol variable, ΔV = 0.12$^m$ |
| CS Vel | | CS | | | 09$^h$ 41$^m$ 10.26$^s$ | −53° 48′ 57.8″ | 11.24 | | | | in Ruprecht 79; classical Cepheid, V$_{max}$ = 11.24$^m$, V$_{min}$ = 12.21$^m$, P = 5.90 d |
| LSS 2018 | | KV | | | 10$^h$ 54$^m$ 40.57$^s$ | −48° 47′ 02.9″ | 12.12 | | | O | central star of DS 1; re-radiating spectroscopic binary, V$_{max}$ = 11.78$^m$, V$_{min}$ = 12.34$^m$, P = 0.36 d |
| WASP-19 | | | | | 09$^h$ 53$^m$ 40.08$^s$ | −45° 39′ 33.1″ | 12.3 | 5.3 | 815 | G8V | has a transiting planet (b) |
| GRS 1009-45 | | MM | | | 10$^h$ 13$^m$ 36.38$^s$ | −45° 04′ 32.0″ | 14.71 | | | G5V-M0V | X-ray nova |
| V382 Vel | | V382 | | | 10$^h$ 44$^m$ 48.39$^s$ | −52° 25′ 30.7″ | 16.6 | | | | nova, V$_{max}$ = 2.8$^m$, V$_{min}$ = 16.6$^m$, P = 0.16 d |
| RX J0925.7-4758 | | MR | | | 09$^h$ 25$^m$ 46.00$^s$ | −47° 58′ 17.4″ | 16.98 | | | | close binary supersoft source, V$_{max}$ = 16.98$^m$, V$_{min}$ = 17.3$^m$, P = 4.03 d |
| CU Vel | | CU | | | 08$^h$ 58$^m$ 33.03$^s$ | −41° 47′ 51.7″ | 17.0 | | | | SU UMa variable, V$_{max}$ = 10.5$^m$, V$_{min}$ = 17.0$^m$, P = 0.079 d |
| 2S 0918-549 | | | | | 09$^h$ 20$^m$ 26.47$^s$ | −55° 12′ 24.5″ | 21.0 | | | | low-mass X-ray binary |
| HH 46 IRS | | | | | 08$^h$ 25$^m$ 43.85$^s$ | −51° 00′ 32.6″ | | | | | in HH 46; young stellar object |
| PSR B1055-52 | | | | | 10$^h$ 57$^m$ 58.84$^s$ | −52° 26′ 56.3″ | | | | | pulsar |
| PSR J0855-4644 | | | | | 08$^h$ 55$^m$ 36.18$^s$ | −46° 44′ 13.4″ | | | | | pulsar; possibly associated with the Vela supernova remnant |
| Vela Pulsar | | HU | | | 08$^h$ 35$^m$ 20.66$^s$ | −45° 10′ 35.2″ | 23.6 | | 959 | | pulsar; associated with the Vela supernova remnant |
| Luhman 16 | | | | | 10$^h$ 49$^m$ 18.92$^s$ | −53° 19′ 10.1″ | | | 6.6 | L7.5+T0.5 | brown dwarf; one of the closest known systems |
| 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.] ||||||||||||