Kataloge

Puppis / Yale Bright Star Catalog (HR)

«Yale Bright Star Catalogue, 5th Revised Ed.» Hoffleit D., Warren Jr W.H., 1991 [154]
HR B F DM HD SAO FK5 IR M* ADS VarID RA Dec vMag spType dMag Sep Remarks
HR 2157 CD-45 2300 41700 217702 231 W C 06 04 28.4 -45 02 12 6.35 G0IV-V 0.3 196.7 D:CPM with HR 2158.
HR 2158 CD-45 2302 41742 217706 W AB 06 04 40.2 -45 04 44 5.93 F4V 0.3 196.7 D:Binary 5.9, 9.4v sep. 5", CPM with HR 2157.,DYN:0.046".
HR 2162 CD-48 2124 41824 217708 W 2827 06 04 46.9 -48 27 31 6.58 G6V 0.3 2.5 D:7.2 G5, 7.4, 463.5y, a = 2.94".,DYN:0.037".,RV:Component B, +14k/s and vsini 2.3k/s.,VAR:Amp. 0.10V. Component A is itself double, showing variable radial velocity 12.10 to 33.22k/s, and vsini 7.99k/s. One,VAR:of the three components may be a spotted star.
HR 2178 CD-45 2317 42168 217724 06 07 01.9 -45 05 29 6.51 K1III
HR 2187 CD-44 2452 42448 217735 W 06 08 34.6 -44 21 22 6.27 B8II 6.8 33.1
HR 2204 CD-49 2084 42683 217747 06 09 23.3 -49 33 46 6.49 F7V
HR 2211 CD-45 2349 42834 217758 2472 06 10 39.9 -45 16 55 6.31 A0V
HR 2281 CD-50 2169 44362 234442 06 18 46.8 -50 21 33 7.04 G2Ib
HR 2290 CD-48 2259 44594 217861 2486 I 06 20 06.1 -48 44 28 6.60 G3V
HR 2348 CD-48 2308 45572 217922 W 06 25 43.6 -48 10 38 5.76 B9V 2.5 1.2
HR 2384 CD-50 2241 46273 234539 W 06 29 49.1 -50 14 21 5.27 F2V 0.1 0.5 D:Quadruple system, AB 6.1 G5, 6.2, 52.9y, a = 0.484". CoD = -50d2440, 9.7, 9.8v sep. 0.5" at 12" from AB, 105.6y, a =,D:0.535". AB, CD are CPM.,DYN:AB, 0.022"; CD, 0.020".
HR 2451 ν CD-43 2576 47670 218071 252 3062 06 37 45.7 -43 11 46 3.17 B8III G:Member of Pleiades group.,VAR:Beta C?, 3.16 - 3.20V.
HR 2462 CD-48 2417 47973 218093 W 3072 06 38 37.6 -48 13 13 4.93 G8III 2.3 13.0 D:Binary. Companion A0.,DYN:0.010".,N:Becvar calls this Y Pup; Lacaille called it V Pup, but it is neither of the variables now known as either V or Y.,VAR:5.58 - 5.62p.
HR 2465 CD-38 2817 48087 197064 06 39 56.9 -38 09 32 6.58 K1IIICNIb
HR 2475 CD-40 2625 48383 218126 W 06 41 14.1 -40 20 59 6.12 B4V 3.4 15.4 D:Companion has A-type spectrum.
HR 2476 CD-47 2521 48403 218124 06 40 49.3 -47 40 29 6.65 M2III
HR 2482 CD-38 2844 48543 197108 W 06 42 16.4 -38 23 55 6.29 A3V+F/G 1.5 7.9 S:Also classified A5:m.
HR 2488 CD-39 2798 48797 197134 2519 06 43 23.3 -39 11 36 6.30 A8:mDel Del S:Also classified A7/9 + F/G:
HR 2507 CD-39 2831 49319 197192 06 46 03.3 -39 32 24 6.62 B6Vnne S:Weak double emission in H beta, H gamma, H delta.
HR 2510 CD-37 3065 49336 197195 V339 Pup 06 46 12.1 -37 46 32 6.21 B4Vne G:Sco-Cen assoc.,VAR:Gamma Cas 6.15 - 6.27V. A 2-year (1977-78) minimum attributed to a dust cloud.
HR 2518 CD-37 3080 49591 197215 1178 W 06 47 21.4 -37 55 47 5.26 B9IV 5.8 65.4
HR 2546 CD-45 2773 50196 218236 W 3236 06 49 57.8 -45 27 00 6.55 K5-M0III 4.6 6.6 VAR:6.52 - 6.57V.
HR 2548 CD-46 2703 50223 218235 2529 06 49 54.6 -46 36 53 5.14 F5V N:Called X Pup by Lacaille, but is not the variable now known as X.
HR 2549 CD-34 3140 50235 197277 06 50 52.4 -34 22 02 4.99 K5III
HR 2553 τ CD-50 2415 50310 234735 263 06 49 56.2 -50 36 53 2.93 K1III SB:1066.0d, K 4.1k/s, V0 +36.4k/s, asini 59.9. Unresolved by speckle interferometry 1980.02.
HR 2558 CD-36 3189 50445 197291 06 51 42.3 -36 13 49 5.96 A3V
HR 2563 CD-48 2556 50621 218261 06 51 32.8 -48 17 33 6.42 K2-3III
HR 2575 CD-42 2793 50785 218272 06 52 39.7 -42 30 16 6.52 F5II-III
HR 2579 CD-43 2756 50860 218278 W 06 52 47.1 -43 58 33 6.46 B8V 6.0 10.0
HR 2591 CD-42 2818 51208 218296 2534 NP Pup 06 54 26.7 -42 21 56 6.32 C3II VAR:Lb 6.25 - 6.37V.
HR 2594 CD-50 2458 51266 234774 06 54 02.3 -50 36 42 6.26 K0-1III
HR 2604 CD-35 3225 51682 197388 06 56 45.7 -35 20 30 6.29 K2III
HR 2608 CD-48 2601 51799 218324 06 56 16.0 -48 43 16 4.95 M1III
HR 2612 CD-35 3233 51825 197402 W 06 57 17.6 -35 30 27 6.23 F8IV-V 0.2 0.2 D:6.9 F8IV-V, 7.1 F8IV-V, 16.74y, a = 0.218". Combined mag., colors.,DYN:0.037".
HR 2619 CD-33 3389 52092 197427 2541 06 58 25.1 -34 06 42 5.06 B3V
HR 2626 CD-45 2850 52362 218360 06 58 41.8 -45 46 05 6.22 A0V G:NGC 129.,SB:Small RV amp. Secondary fainter.
HR 2641 CD-33 3415 52703 197475 07 00 49.8 -33 27 55 6.40 G8II-III
HR 2658 CD-43 2882 53253 218396 07 02 15.6 -43 24 15 6.43 A0V
HR 2666 CD-42 2929 53704 218424 1184 Var? 07 04 02.8 -42 20 14 5.20 Am G:Hyades moving group.,S:K/m indicate A3/F2, respectively.,VAR:5.16 - 5.32V.
HR 2667 CD-43 2906 53705 218421 I W A 07 03 57.3 -43 36 29 5.54 G3V 1.2 21.0 D:CPM with HR 2668 and third component, 9.2v K2 at 200".
HR 2668 CD-43 2907 53706 218423 I W B 07 03 58.8 -43 36 42 6.79 K0V 1.2 21.0 D:See HR 2667.
HR 2672 CD-49 2587 53811 218427 07 03 53.7 -49 35 02 4.93 A4IV G:Hyades group.
HR 2677 CD-34 3327 53952 197557 W 07 05 32.0 -34 46 40 6.14 F2V 1.3 3.1 D:AB binary A9V, F6V. CPM with C, 10.0v at 37".
HR 2685 CD-38 3163 54153 197572 07 06 02.3 -38 22 58 6.11 G0IIaCH1
HR 2687 CD-50 2561 54179 234907 07 05 16.5 -50 21 37 6.46 K3III
HR 2691 CD-40 2930 54475 218465 Var 07 07 07.1 -40 53 36 5.79 B3V t S:Also classified B9e.,VAR:Amp. 0.02V, 0.04U. Var. H alpha emission.
HR 2702 CD-39 3105 54893 197632 2551 3431 07 08 51.1 -39 39 21 4.83 B2IV-V G:Member of a possible association in the anticenter direction at about 250pc, including HR 2756, 2961, 3330, 3440, 3466,,G:3467, 3663, 3672, and 3674.,VAR:Beta C?
HR 2719 CD-48 2765 55526 218514 2554 07 10 47.5 -48 55 56 5.14 K2III G:61 Cyg group.
HR 2726 CD-36 3421 55718 197694 W 3464 07 12 25.7 -36 32 40 5.96 B3V 2.5 2.5 VAR:The fainter component of the double is the variable suspect, 7.5v.
HR 2727 CD-40 2987 55719 218525 Var? 07 12 15.8 -40 29 56 5.31 A3pSrEuCr S:Strong Ap star.,SB:46.314d, K 48.5k/s, V0 -4.4k/s, asini 30.6.,VAR:Magnetic field var. 36.5d.
HR 2740 CD-46 2977 55892 218537 275 QW Pup 07 12 33.6 -46 45 34 4.49 F0IV VAR:Amp. about 0.07u, 0.04v, 0.02b, 0.04y; 0.936d.
HR 2746 CD-44 3223 56022 218546 OU Pup 07 13 13.4 -45 10 59 4.89 A0pSi VAR:Amp. about 0.04u, 0.01v,b,y. Combining their data with previous observations, Heck et al. (1987, A&AS, 70, 33),VAR:derive 0.91889d.
HR 2748 CD-44 3227 56096 218549 W L2 Pup 07 13 32.4 -44 38 23 5.10 M5IIIe 6.4 62.0 C:IR source.,S:SiO maser.,VAR:Primary of vis. double, SRb 2.6 - 6.2v, 140.42d.
HR 2759 CD-41 2906 56410 218568 07 14 57.1 -41 25 33 5.94 B4III-IV
HR 2761 CD-46 3000 56455 218570 PR Pup 07 14 45.9 -46 50 59 5.72 A0pSi VAR:Amp. 0.04y, 1.93d.
HR 2762 CD-48 2807 56456 218567 W 07 14 38.2 -48 16 18 4.76 B8-9V 8.6 18.5 D:Companion optical.
HR 2769 CD-38 3288 56733 197785 07 16 31.8 -38 19 08 5.80 B4V RV:Published values range fron -3 to +45k/s.
HR 2770 CD-36 3485 56779 197790 Var? 07 16 49.5 -36 35 34 5.03 B2IV-V G:Ori OB1.
HR 2771 CD-46 3023 56813 218589 07 16 15.5 -46 46 28 5.66 K4III
HR 2773 π CD-36 3489 56855 197795 278 W 3515 07 17 08.6 -37 05 51 2.70 K3Ib 5.3 69.2 G:In cluster Collinder 135, but too bright to be member.,S:Also classified K4III. IUE observations suggest an early-type companion.
HR 2787 CD-36 3512 57150 197824 W NV Pup 07 18 18.4 -36 44 03 4.66 B2V+B3IVne 0.4 239.9 S:Shell star. Strong H alpha and FeII emission.,VAR:Amp. 0.18V.
HR 2789 CD-43 3093 57197 218618 07 18 04.2 -43 59 12 5.85 B8II-III
HR 2790 CD-36 3519 57219 197837 NW Pup 07 18 38.2 -36 44 34 5.11 B2IVne VAR:Beta C amp. 0.02V. 3-hour period not confirmed. Ell, amp. 0.045V, 1d.
HR 2791 CD-38 3309 57240 197836 07 18 33.6 -39 12 37 5.25 A1V
HR 2794 CD-33 3696 57299 197842 2566 07 19 13.7 -33 43 38 6.30 K2-3III
HR 2829 CD-35 3569 58420 197951 W 07 23 58.3 -35 50 16 6.31 B7III 6.2 25.0 D:Companion F5V, optical.
HR 2842 CD-37 3549 58634 197974 W B 07 24 47.2 -37 17 24 6.97 F0V: 0.1 7.0 D:Combined mag. and colors with HR 2843, 6.15V, +0.25(B-V), +0.15(U-B).
HR 2843 CD-37 3549 58635 197975 W A 07 24 47.3 -37 17 27 6.84 F0V: 0.1 7.0 D:See HR 2842.
HR 2856 CD-33 3813 59026 198000 07 26 42.3 -34 08 27 5.90 B2IV-V
HR 2860 BD-22 1878 59136 173778 07 27 42.9 -22 51 35 5.95 B5V:
HR 2863 CD-28 4383 59256 173799 Var? 07 27 59.2 -29 09 21 5.54 B9VpSi:
HR 2868 BD-14 1925 59438 152943 6126 07 29 21.9 -14 59 57 6.05 F7V 1.4 2.2 D:AB 6.4 F4V, 7.5, 1090.9y, a = 3.684". C, 11.5v M0 at 21" orbital period around AB probably over 10000y. Component D,,D:12v at 42" optical?,DYN:0.033".
HR 2869 CD-37 3601 59466 198031 07 28 22.8 -37 48 37 6.58 A1IV
HR 2870 CD-31 4590 59499 198038 W A 07 28 51.3 -31 50 54 6.38 B3V 0.7 8.9 D:Mag. and colors for combined HR 2870-1, 5.94V, -0.16(B-V), -0.67(U-B).
HR 2871 CD-31 4590 59500 198039 W B 07 28 51.5 -31 50 49 7.13 B4V 0.7 8.9
HR 2873 CD-31 4593 59550 198042 07 29 04.9 -31 27 23 5.77 B2V
HR 2874 BD-22 1897 59612 173864 W 07 29 51.4 -23 01 28 4.85 A5Ib 5.9 3.0
HR 2875 CD-38 3400 59635 198045 2580 07 29 05.7 -38 48 44 5.43 B5Vp
HR 2878 σ CD-43 3260 59717 218755 1194 W 07 29 13.8 -43 18 05 3.25 K5III 5.3 22.3 D:CPM. Companion G5V.,G:Sigma Pup group.,SB:Primary of visual double, 257.8d, K 18.6k/s, V0 +87.3k/s, asini 65.0.
HR 2881 CD-30 4620 59890 198064 I 07 30 42.5 -30 57 44 4.65 G3Ib
HR 2882 CD-37 3637 59967 198069 I 07 30 42.4 -37 20 23 6.65 G4V
HR 2885 CD-35 3650 60098 198086 3629 07 31 25.8 -36 09 10 6.68 B4V
HR 2889 CD-35 3652 60168 198093 W PS Pup 07 31 42.8 -35 53 16 6.61 A0V 4.4 91.5 VAR:Ell amp. 0.051u, 0.03v, b, y. 0.6711d. Sp. period revolution about 1.4d.
HR 2895 CD-35 3659 60312 198104 W 07 32 22.3 -35 57 41 6.30 B9V 1.2 0.3
HR 2897 BD-14 1966 60325 153061 07 33 22.1 -14 20 18 6.21 B1V G:NGC 2422.
HR 2899 BD-19 1944 60341 153062 07 33 19.5 -19 24 45 5.66 K3III G:Wolf 630 group.
HR 2900 CD-24 5566 60345 173987 07 33 09.7 -24 42 39 5.85 A7V:
HR 2902 BD-14 1971 60414 153072 I KQ Pup 07 33 47.9 -14 31 26 4.97 M2Iabpe+B2V v G:NGC 2422 #9.,M:Rapidly evolving shell.,SB:9752d, K 17.1k/s, V0 +34.4k/s, asini 2040. Unresolved by speckle interferometry 1980.02, 1983.11. SKYLAB indicates,SB:cool star with hot companion. Tenuous gas enveloping both stars.,VAR:VV Cep type or symbiotic, 4.88 - 5.17V. Var. shell spectrum.
HR 2906 BD-21 2007 60532 174009 288 07 34 03.2 -22 17 46 4.45 F6IV G:Zeta Her group.
HR 2907 CD-39 3398 60559 198120 07 33 13.5 -40 03 32 6.26 B8IVpSi
HR 2908 CD-42 3325 60574 218792 07 33 13.3 -43 05 11 6.52 G8III
HR 2909 CD-23 5709 60584 174019 6190 A 07 34 18.6 -23 28 25 5.83 dF4 0.0 9.6 D:Binary with HR 2910. Colors for combined light. Magnitude of blended images 5.09V.,DYN:0.029".
HR 2910 CD-23 5709 60585 174020 6190 B 07 34 19.1 -23 28 29 5.87 dF6 0.0 9.6 D:See HR 2909.,DYN:0.029".
HR 2911 CD-36 3715 60606 198130 OW Pup 07 33 51.0 -36 20 18 5.54 B3Vne S:Shell star.,VAR:5.5 - 5.60B. Also amp. 0.025 on time scale of 2d reported.
HR 2912 CD-25 4719 60629 174028 07 34 28.8 -26 07 00 6.65 A0V
HR 2913 CD-33 3926 60646 198138 07 34 12.8 -33 27 48 6.11 A9IV
HR 2916 CD-26 4574 60666 174033 07 34 34.9 -27 00 43 5.77 K1III
HR 2917 CD-39 3407 60686 198137 07 33 58.5 -39 54 21 6.76 K2III
HR 2921 BD-14 1999 60855 153118 6208 Var 07 36 03.9 -14 29 34 5.70 B2Ve 3.8 19.6 D:AB fixed; B, 12.2v at 5". C, 9.71V, +0.03(B-V), -0.23(U-B), B9.5V, optical?,G:In cluster NGC 2422 #45.,VAR:Amp. at 0.58 micrometers about 0.10m.
HR 2922 CD-28 4566 60863 174058 6205 07 35 22.8 -28 22 10 4.64 B8V 4.5 38.4 D:Companions optical. C is G type, strong lithium.
HR 2923 BD-21 2030 60951 174092 07 36 07.8 -22 09 38 6.34 G5
HR 2928 BD-19 1967 61068 153149 1197 PT Pup 07 36 41.0 -19 42 08 5.74 B2III VAR:Amp. 0.01B, 0.16121d.
HR 2932 BD-14 2053 61224 153172 W 07 37 38.9 -14 26 28 6.53 B9IIIe 2.8 65.0 G:NGC 2422 #125.,S:Shell star.
HR 2933 CD-23 5791 61227 174141 07 37 16.8 -23 46 30 6.37 F0II
HR 2937 CD-34 3755 61330 198195 290 W 07 37 22.1 -34 58 07 4.53 B8IV 0.5 0.1 D:Triple system, components all about same mag. and within about 1".
HR 2940 CD-48 3069 61391 218841 2591 07 36 43.9 -48 49 49 5.72 B9.5V
HR 2942 CD-34 3760 61409 198205 07 37 44.8 -35 16 38 6.60 K1III
HR 2944 CD-25 4828 61429 174175 6246 PU Pup 07 38 18.0 -25 21 53 4.70 B8IV 0.4 0.2 D:Unresolved by speckle interferometry.,N:m Pup. Originally called Pi in Bayer and Argelander. Called m in Lacaille (1763) and Baily. Another star HR 2773,,N:also called Pi in Argelander, is the currently accepted star of this designation.,VAR:EW amp. 0.06V, 2.57895d.
HR 2945 CD-37 3736 61453 198210 07 37 45.2 -38 00 38 6.38 K4III G:Region of NGC 2451.
HR 2947 BD-18 1946 61554 153195 07 39 07.1 -18 40 45 6.72 B6Vn
HR 2948 CD-26 4707 61555 174198 6255 A 3673 07 38 49.3 -26 48 06 4.50 H B6V 0.2 9.9 D:Binary with HR 2949 at 10". C, 13.8v at 6" optical. Colors for combined light AB. Combined mag. 3.82V.,N:Markab; Markeb. Sometimes called Kappa or Kappa1, sometimes k, k1 or k3 Pup. However, HR 2873 and,N:2881 have also been variously designated as k, k1, k2 or k3 Pup.
HR 2949 CD-26 4707 61556 174199 6255 B 3673 07 38 49.8 -26 48 13 4.62 H B5IVn 0.2 9.9 D:See HR 2948.,N:Frequently designated as k2 Pup, or Kappa2.
HR 2952 CD-39 3463 61623 198226 07 38 24.2 -39 59 29 6.59 A0
HR 2954 CD-36 3773 61641 198237 07 38 43.9 -36 29 49 5.80 B2IV-V N:Called e in Lacaille, BAC. However, Bayer and Argelander called HR 3102 e; 3102 later changed to j Pup.
HR 2955 CD-38 3521 61642 198229 07 38 32.6 -38 46 52 6.19 G8III G:Region of NGC 2451 (#163).
HR 2956 CD-26 4722 61672 174219 07 39 26.9 -26 51 47 6.50 B7V
HR 2957 CD-48 3091 61715 218852 MY Pup 07 38 18.2 -48 36 04 5.68 F4Iab VAR:CDelta 5.54 - 5.76V, 5.6952d.
HR 2959 BD-14 2082 61772 153227 I 07 40 23.2 -15 15 49 4.94 K3II
HR 2960 BD-19 2003 61774 153225 6273 07 40 13.6 -19 39 39 5.93 K0 5.2 8.3 D:Optical.
HR 2961 CD-38 3531 61831 198253 07 39 27.4 -38 18 30 4.84 B2.5V G:NGC 2451 #175; probable member. See HR 2702.
HR 2963 CD-37 3767 61878 198265 W 07 39 43.8 -38 08 22 5.73 B5Vn 2.7 1.1 G:NGC 2451 #182; probable member. See HR 2702.
HR 2964 CD-37 3768 61899 198268 07 39 47.8 -38 15 39 5.76 B2.5V G:NGC 2451 #184.
HR 2968 CD-37 3770 61925 198273 07 39 58.0 -37 34 46 6.00 B6IVe G:NGC 2451 #187.
HR 2972 CD-27 4393 61987 174273 07 40 43.4 -27 56 45 6.76 B3-5IV-V:
HR 2974 CD-31 4910 62058 198286 R Pup 07 40 52.7 -31 39 39 6.56 G20-Ia G:Probable member and brightest star in open cluster NGC 2439; possible member of Pup OB1.,VAR:SRd? 6.56 - 6.64V, over 27d. Discovered by Gould 1879, variability questioned. Now confirmed by PEP observations, amp.,VAR:0.19U, larger in V.
HR 2976 BD-21 2077 62082 174298 I 07 41 23.6 -22 20 14 6.18 M1III
HR 2981 CD-38 3556 62226 198298 07 41 15.8 -38 32 01 5.42 B5V G:NGC 2451 #203.
HR 2984 CD-44 3655 62318 218905 07 41 21.8 -44 37 56 6.41 B7IV-V
HR 2986 CD-38 3564 62376 198315 07 41 58.0 -38 31 44 6.54 B7V
HR 2988 CD-26 4824 62412 174356 07 42 48.1 -26 21 04 5.64 K1III
HR 2992 CD-25 4966 62555 174395 W 07 43 39.1 -25 30 14 6.55 A3 7.5 5.3
HR 2993 1 CD-28 4767 62576 174391 I 6324 3708 07 43 32.4 -28 24 40 4.59 K3Ib 8.9 26.2
HR 2994 CD-35 3809 62578 198343 07 43 12.0 -36 03 01 5.60 B5V
HR 2995 CD-38 3583 62595 198342 07 43 07.0 -38 51 51 6.89 G6/8III
HR 2996 3 CD-28 4774 62623 174400 2601 I 07 43 48.5 -28 57 17 3.96 A2Iabe C:Infrared color excess. Color excess E(B-V) = +0.13.,N:Called Tau in Argelander, Bayer, HP 1462, (but now Tau is HR 2553). HR 2996 called l in HR 50 and Lacaille,N:1763.,SB:137.767d, K 3.6k/s, V0 +25.4k/s, asini 6.53.,VAR:Var. in red and IR. Amp. 0.24R, 0.20(R-I).
HR 2998 CD-44 3675 62644 218923 07 42 57.2 -45 10 24 5.06 G6IV
HR 3001 CD-37 3820 62712 198352 07 43 42.9 -38 12 07 6.40 B9VpSi G:NGC 2451 #233.
HR 3002 CD-40 3377 62713 218932 2603 07 43 41.9 -40 56 02 5.17 K1III N:Called W by Lacaille (1763), but it is not the variable now named W Pup.
HR 3004 CD-24 5885 62747 174433 Var? 07 44 34.0 -24 40 26 5.62 B1.5III G:Sco-Cen assoc.,VAR:Amp. 0.07b?
HR 3005 CD-49 3014 62756 218928 07 43 06.9 -49 59 34 6.57 A2V
HR 3007 CD-35 3825 62781 198366 07 44 09.6 -36 03 46 5.80 F2V
HR 3009 2 BD-14 2193 62863 153362 6348 B PV Pup 07 45 28.7 -14 41 10 6.89 A8V 0.8 16.8 D:Binary with HR 3010.,VAR:E, amp. 0.41y, 1.660d. Equal components.
HR 3010 2 BD-14 2194 62864 153363 6348 A 07 45 29.1 -14 41 27 6.07 A2V 0.8 16.8 D:Binary with HR 3009.
HR 3011 CD-37 3841 62893 198379 07 44 34.2 -37 56 35 5.88 B7V G:NGC 2451 #246.
HR 3015 4 BD-14 2199 62952 153372 1202 07 45 56.9 -14 33 50 5.04 F0V
HR 3016 CD-37 3861 62991 198390 07 45 04.6 -37 53 16 6.54 B3IV G:NGC 2451 #251.
HR 3017 CD-37 3863 63032 198398 2605 3723 07 45 15.3 -37 58 07 3.61 K2.5Ib-II G:NGC 2451 #254; membership questioned.,N:Called c Pup in Argelander, Norton and most modern catalogues, this was originally called b Pup by Lacaille (1763).
HR 3018 CD-33 4113 63077 198404 07 45 35.0 -34 10 23 5.37 G0V S:Metal deficient.
HR 3019 BD-12 2135 63112 153389 07 46 44.9 -12 40 31 6.39 A0V
HR 3020 CD-43 3534 63118 218955 07 45 18.1 -43 45 08 6.03 B6IV
HR 3022 CD-37 3886 63215 198416 07 46 10.4 -37 56 02 5.88 B7V t G:NGC 2451 #267.,VAR:H alpha emission var.
HR 3023 BD-22 2027 63271 174533 Var? 07 47 12.5 -22 31 11 5.90 B2IV-V VAR:Amp. 0.03b.
HR 3025 CD-39 3587 63308 198424 07 46 33.4 -40 03 35 6.57 B2V G:Member of the local association (Pleiades group).
HR 3026 BD-15 2049 63302 153404 QY Pup 07 47 38.5 -15 59 27 6.34 K1Ia-Iab VAR:Amp. 0.2V.
HR 3027 BD-15 2052 63323 153409 I W 3741 07 47 45.2 -16 00 52 6.43 M2II-III 0.1 130.5 VAR:Amp. 0.18V.
HR 3029 5 BD-11 2106 63336 153414 6381 07 47 56.7 -12 11 35 5.48 dF5 1.8 2.0 D:Binary. Companion dG3.
HR 3032 CD-39 3595 63401 198435 OX Pup 07 47 05.8 -39 19 53 6.31 B8III G:Region of NGC 2451.,VAR:2.41d, 0.06V.
HR 3034 ο CD-25 5081 63462 174558 6384 3745 07 48 05.2 -25 56 14 4.50 B0V:pe: v 8.0 27.0 S:Also classified B1IVe. Small variations in H alpha.,VAR:SR? Amp. about 0.02V. R-I also found at +0.06 and +0.07.
HR 3035 CD-38 3650 63465 198442 W 07 47 25.0 -38 30 40 5.08 B2.5III 5.8 10.9 G:NGC 2451 #283.
HR 3037 CD-46 3435 63578 219000 1203 07 47 31.5 -46 36 31 5.23 B1.5IV
HR 3041 CD-40 3490 63640 219006 T Pup 07 48 08.5 -40 39 08 6.14 M2III VAR:Cst 6.14V.
HR 3042 BD-12 2164 63655 153449 07 49 28.6 -13 21 12 6.23 B8III
HR 3043 CD-24 6022 63660 174592 07 49 01.7 -24 54 44 5.33 G0III
HR 3044 6 BD-16 2146 63697 153454 2607 I 07 49 41.2 -17 13 42 5.18 K3III
HR 3045 ξ 7 CD-24 6030 63700 174601 1204 I 6393 07 49 17.7 -24 51 35 3.34 G6Iab-Ib 9.5 5.1 N:Azmidiske; Asmidiske, a name more properly applied to HR 3699 according to Allen.,S:Also classified G3Ib.
HR 3046 CD-46 3451 63744 219018 07 48 20.3 -47 04 40 4.71 K0III
HR 3048 BD-19 2085 63754 174617 6398 07 49 45.2 -20 12 25 6.56 G3V 7.0 6.0
HR 3049 CD-34 3970 63786 198480 3756 07 49 14.7 -35 14 36 5.93 B9V SB:Large amp. Secondary fainter and later Sp.,VAR:Amp. 0.5p.
HR 3051 BD-19 2089 63822 153468 07 50 05.7 -19 31 25 6.12 K0
HR 3052 CD-32 4451 63852 198487 2608 07 49 35.4 -33 17 20 5.60 K5III
HR 3055 CD-46 3458 63922 219035 W 07 49 14.3 -46 22 24 4.11 B0III 4.9 59.2 D:Companion B9V, RV -72k/s, optical.
HR 3057 CD-44 3762 63948 219040 07 49 28.2 -44 45 07 6.32 K0III
HR 3058 CD-46 3460 63949 219034 QS Pup 07 49 12.9 -46 51 28 5.84 B1.5IV VAR:Beta C, amp. 0.015u, 0.1182d.
HR 3060 CD-24 6060 64042 174658 6414 07 51 00.0 -24 31 42 6.45 A0 3.5 0.9
HR 3063 8 BD-12 2179 64077 153499 07 51 40.9 -12 49 10 6.36 F2
HR 3064 9 BD-13 2267 64096 153500 6420 07 51 46.3 -13 53 53 5.17 G0V: 0.7 0.4 D:5.6 F9V, 6.2 G4V, 23.18y, a = 0.58". Combined mag., colors. Masses 0.86 and 0.99 solar.,DYN:0.057".,G:UMa stream.,SB:8467d, K 4k/s, V0 -21.2k/s, asini 337. Speckle interferometric sep. 0.170", 1980.94; 0.273", 1983.11.
HR 3068 BD-20 2235 64152 174679 07 51 42.9 -21 10 26 5.63 G8III G:Probable Hyades group.
HR 3069 CD-44 3780 64181 219059 07 50 42.4 -44 34 47 6.45 G6III
HR 3071 CD-50 3004 64225 235552 07 50 23.9 -50 30 35 5.91 K2III
HR 3073 10 BD-14 2250 64238 153520 07 52 18.9 -14 50 47 5.69 F1Ia
HR 3074 CD-42 3601 64287 219069 07 51 20.5 -43 05 44 6.32 B2IV-V
HR 3078 CD-42 3610 64365 219076 QU Pup 07 51 40.3 -42 53 18 6.04 B2IV G:Member of the local association (Pleiades group).,RV:Amp. about 10k/s, probably same period as light variation.,VAR:BetaC, Amp. 0.03b, 0.040u with large modulation. Primary period 0.1927d with secondary 0.1680 or 0.2019d.
HR 3079 CD-34 4036 64379 198540 W 07 52 15.7 -34 42 19 5.01 F5V 3.6 3.0 D:Binary.,DYN:0.021".,G:Hyades group?
HR 3080 CD-40 3579 64440 219082 301 07 52 13.0 -40 34 33 3.73 K1-2II+A0 N:a Puppis, often misnamed alpha.,SB:2660d, K 11.8k/s, V0 +24.0k/s, asini 396. Unresolved by speckle interferometry 1978.96, 1980.02. SKYLAB UV spectra,SB:spectra indicate cool star with hot subdwarf or white dwarf companion.
HR 3084 CD-38 3769 64503 198545 QZ Pup 07 52 38.7 -38 51 47 4.49 B2.5V G:Near open cluster NGC 2477.,N:Called b Pup in Argelander and most modern catalogues. Was originally called a Pup by Lacaille (1763).,VAR:Beta C or Ell?, 4.47 - 4.54V, amp. 0.07y.
HR 3085 CD-36 3989 64572 198553 07 53 03.5 -36 21 50 5.43 K0III
HR 3089 CD-49 3137 64740 219106 07 53 03.7 -49 36 47 4.63 B1.5Vp v M:Located just inside 3U0750-49 error-box.,S:Helium-rich star, nitrogen enhanced.,VAR:HeI 4026 varies, 1.3295d.
HR 3090 CD-47 3396 64760 219111 07 53 18.2 -48 06 11 4.24 B0.5Ib N:Early catalogues (Lacaille 1763) called this star R but it is not the var. now named R Pup. Re-named J Pup.,S:Unusually large line-broadening for luminosity Ib.
HR 3091 CD-35 4002 64802 198575 07 54 11.0 -35 52 39 5.49 B2V G:Member of the local association (Pleiades group).
HR 3092 CD-34 4091 64876 198579 I 07 54 39.9 -34 50 49 6.15 K4III
HR 3096 CD-30 5275 64974 198591 07 55 13.7 -30 55 03 6.44 K4III
HR 3099 CD-29 5189 65183 198609 I PX Pup 07 56 22.8 -30 17 07 6.33 M6III VAR:Amp. 0.42V.
HR 3101 CD-43 3737 65211 219157 W 07 55 46.5 -43 50 42 6.02 B6V 0.2 0.7
HR 3102 11 BD-22 2087 65228 174852 2615 I 07 56 51.5 -22 52 48 4.20 F7II N:See HR 2954.
HR 3107 CD-40 3655 65315 219169 07 56 24.3 -40 44 11 6.78 B2V
HR 3111 CD-42 3717 65442 219186 07 56 57.9 -42 24 22 6.09 K3III
HR 3113 CD-29 5236 65456 198636 1210 3830 07 57 40.1 -30 20 05 4.79 A2V v G:Pleiades group.,N:Called Chi Argo by Argelander. Not named in Lacaille or BAC. Position agrees with Chi in Bayer (Puppis,N:area).
HR 3114 CD-43 3758 65460 219189 07 56 57.9 -43 30 01 5.35 B2.5V
HR 3116 CD-43 3766 65551 219197 2616 W Var 07 57 18.4 -44 06 35 5.09 B2.5IV 8.9 10.0 VAR:Amp. 0.03b?
HR 3118 CD-47 3457 65598 219200 W 07 57 20.0 -47 53 25 6.22 B5V 0.6 0.5
HR 3121 CD-45 3611 65685 219218 07 57 51.8 -45 34 40 5.17 K2III
HR 3123 12 BD-22 2104 65699 174932 I 07 59 05.7 -23 18 38 5.11 cK2 S:BaII star.
HR 3129 CD-48 3349 65818 219226 W V Pup 07 58 14.4 -49 14 42 4.41 B1Vp+B3IV: 5.9 39.2 G:Member of Pleiades group.,S:Also classified B2II-III(n). Possible X-ray source 3U0750-49.,SB:Component A of visual system, 1.4545d. Relative vel. 610k. Probably consists of two ellipsoids in nearly circular orbit,SB:inclined 75d. Matter appears to stream from secondary to primary.,VAR:Comp. A of visual double, EB 4.74 - 5.25p, 1.4544877d, contact binary, equal components.
HR 3131 BD-18 2118 65810 153687 1212 07 59 52.0 -18 23 57 4.61 A2Vn G:Sirius group; UMa stream. Possible Eggen group with HR 63, q.v.
HR 3137 CD-44 3920 65904 219240 07 59 01.8 -45 12 58 5.99 B4V
HR 3140 CD-38 3908 65925 198668 07 59 28.4 -39 17 50 5.24 F5III
HR 3142 CD-49 3243 66005 219249 W A 07 59 12.3 -49 58 36 6.32 B2IV-V 0.0 16.4 D:CPM with HR 3143.
HR 3143 CD-49 3244 66006 219250 W B 07 59 13.4 -49 58 25 6.34 B2IV-V 0.0 16.4 D:CPM with HR 3142.
HR 3146 CD-45 3662 66190 219280 08 00 19.6 -45 27 25 6.61 K1Ib-II
HR 3148 CD-48 3384 66210 219283 08 00 14.9 -48 58 53 6.02 A2V
HR 3151 CD-48 3388 66255 219292 PY Pup 08 00 28.9 -48 52 17 6.12 A0pSi VAR:Amp. 0.04v, 6.82d.
HR 3154 CD-36 4116 66358 198714 08 01 37.4 -37 17 01 5.95 A3IV
HR 3155 CD-36 4120 66435 198725 3872 08 02 06.2 -37 03 02 6.34 M1III VAR:Amp. 0.07(U-B).
HR 3160 CD-32 4766 66598 198743 I W 08 03 04.1 -32 27 50 5.82 K2-3III 3.1 35.1
HR 3162 CD-40 3776 66624 219339 W V336 Pup 08 02 44.8 -41 18 36 5.52 B9pSi 3.2 26.1 D:Fixed sep. Companion 8.77V, +1.30(B-V), +0.07(U-B), M6III, optical. May be Mira-type variable.,G:Member of Pleiades group.,VAR:Amp. >0.022, 2.008d.
HR 3165 ζ CD-39 3939 66811 198752 306 08 03 35.1 -40 00 12 2.25 O5f e C:Color excess E(B-V) = +0.04.,G:In cluster CR 173; in HII region.,M:With HR 3207, appears capable of producing most of the observed ionization of Gum Neb.,N:Naos; Suhail Hadar.,R:Diam. = 0.00041 - 0.00042".,S:Also classified O4f, O4ef and O4I9n)f.,VAR:Change in H alpha emission profile between 1974 and 1976 interpreted as change in rate of mass loss.
HR 3166 CD-42 3832 66812 219355 08 03 29.5 -42 56 55 6.29 G8II S:Possible BaII star.
HR 3168 14 BD-19 2228 66834 153796 08 04 41.5 -19 43 41 6.13 B3III
HR 3170 CD-32 4796 66888 198764 I MZ Pup 08 04 16.2 -32 40 30 5.31 M1Ib VAR:Lc? 5.2 - 5.44V.
HR 3177 CD-33 4525 67243 198791 W 08 05 44.9 -33 34 09 6.14 G1Ib 2.4 22.1 D:Component B, 8.66V, -0.09(B-V), -0.52(U-B), B9IV.
HR 3183 BD-20 2395 67456 175206 W 08 07 18.0 -20 33 17 5.38 A5II 9.2 13.8 D:Companion not confirmed.
HR 3185 ρ 15 CD-23 6828 67523 175217 308 I W Rho Pup 08 07 32.6 -24 18 15 2.81 F6IIpDel Del e 10.9 29.6 N:Called Iota Pup in Argelander's atlas, and in Bayer.,S:High Fe abundance. Violet shifted CaII K emission at some phase of light curve.,SB:0.14088143d over 60 yr. interval.,VAR:Delta Sct 2.68 - 2.78v, 0.14088143d.
HR 3190 BD-19 2262 67751 175250 W 08 08 43.5 -20 21 47 6.36 A7IV 6.6 20.2
HR 3192 16 BD-18 2190 67797 153890 2632 08 09 01.6 -19 14 42 4.40 B5IV
HR 3194 BD-15 2280 67880 153898 6632 08 09 28.5 -16 14 56 5.68 B2.5V 6.7 5.3 D:Companion A5III, optical.,M:Old disk population runaway star.
HR 3195 CD-37 4288 67888 198848 2631 PQ Pup 08 08 37.6 -37 40 53 6.37 B4V e S:H alpha emission.
HR 3196 CD-29 5620 67921 198854 W 08 09 06.7 -30 19 21 6.65 K5III 4.2 1.1
HR 3199 CD-35 4256 67977 198859 08 09 10.2 -35 27 18 6.20 G8III
HR 3202 18 BD-13 2420 68146 153924 2637 W 08 10 39.8 -13 47 57 5.54 F6V 6.7 93. G:Hyades group.
HR 3205 CD-42 3944 68242 219507 W 08 09 47.7 -42 38 26 6.26 B7V 1.1 5.6 D:Components B6V and B9V.,S:Metallic lines strong for He type B8p.
HR 3211 19 BD-12 2385 68290 153942 I 6647 08 11 16.3 -12 55 37 4.72 G9III-IIIb 3.0 71.0
HR 3219 CD-36 4291 68450 198898 W 08 11 01.6 -37 17 32 6.44 O9.5II 7.0 18.0 G:NGC 2546 #682.,S:Also classified O9.7Ib-II.
HR 3225 CD-39 4084 68553 198908 NS Pup 08 11 21.5 -39 37 07 4.45 K3Ib VAR:Lc 4.4 - 4.5V.
HR 3226 CD-42 3979 68601 219569 W 08 11 25.9 -42 59 14 4.75 A5Ib 4.8 25.7
HR 3229 20 BD-15 2324 68752 153993 311 I 08 13 20.0 -15 47 18 4.99 G5II
HR 3230 CD-29 5738 68758 175390 08 12 46.0 -29 54 39 6.52 A1V
HR 3233 CD-37 4394 68862 198942 08 12 51.5 -37 55 28 6.43 A3V G:NGC 2546 #575.
HR 3237 CD-35 4349 68980 198957 MX Pup 08 13 29.6 -35 53 59 4.78 B1.5IIIe v G:Pup OB3.,RV:Probably pole on.,S:Shell star.,VAR:Gamma Cas 4.60 - 4.88V. H alpha variable.
HR 3238 CD-33 4705 69002 198960 W 08 13 41.1 -33 34 09 6.37 K2III 6.7 6.3
HR 3239 CD-31 5742 69080 198972 2644 W 08 14 11.0 -32 08 27 6.06 B1.5V 7.0 29.6
HR 3240 CD-35 4358 69081 198969 W OS Pup 08 13 58.4 -36 19 21 5.08 B1.5IV 0.9 66.9 VAR:4.60 - 4.71p.
HR 3241 CD-35 4360 69082 198970 08 13 58.8 -36 20 28 6.11 B2IV-V G:Pup OB3.,SB:Secondary Sp. later and much fainter.
HR 3242 CD-35 4365 69123 198979 08 14 13.2 -35 29 26 5.78 K1III
HR 3243 CD-39 4128 69142 219635 W 08 14 02.9 -40 20 53 4.44 K1II-III 5.1 51.1 SB:930d, K 10.8k/s, V0 +13.5k/s, asini 127.
HR 3251 CD-30 5946 69445 199010 W 08 15 52.5 -30 55 33 6.21 G5-8III+G: 1.9 2.2
HR 3253 CD-35 4401 69511 199015 08 15 58.9 -35 54 10 6.16 K2III
HR 3255 BD-20 2467 69589 175497 08 16 54.2 -21 19 13 6.60 A0
HR 3257 21 BD-15 2362 69665 154076 3986 08 17 23.1 -16 17 06 6.16 A2V
HR 3259 BD-12 2449 69830 154093 08 18 23.9 -12 37 55 5.98 G7.5V
HR 3261 CD-29 5897 69879 175543 08 17 58.3 -30 00 12 6.45 K0III
HR 3266 CD-35 4452 70002 199061 08 18 17.4 -35 27 06 5.58 K2III
HR 3267 CD-36 4443 70003 199059 W 08 18 12.6 -37 22 27 6.70 A0IV+G: 0.8 1.9 SB:Brighter component of visual double.
HR 3270 CD-36 4449 70060 199070 313 08 18 33.3 -36 39 34 4.45 A7III
HR 3273 CD-34 4627 70235 199084 08 19 29.4 -34 35 25 6.43 B9pHgMn S:Also classified B8Ib/II.
HR 3276 BD-22 2233 70302 175634 W 08 20 27.4 -22 55 29 6.13 K0 7.0 6.7
HR 3279 BD-19 2369 70442 154150 2647 08 21 21.2 -20 04 45 5.58 G2III+A3 G:Sirius group; UMa stream.,S:Also classified G8III + A0:V.,SB:Unresolved by speckle interferometry. vsini of A3 component 80k/s.
HR 3281 BD-17 2464 70523 154159 08 21 54.6 -17 35 11 5.75 K1III G:Zeta Her group.
HR 3282 CD-32 5185 70555 199118 1219 I 08 21 23.0 -33 03 16 4.83 K2.5II-III
HR 3283 CD-36 4513 70556 199119 W 08 21 21.0 -36 29 04 5.20 B2IV-V 6.8 6.8 D:Companion A2V, optical.
HR 3286 CD-39 4245 70612 199123 2648 08 21 24.2 -39 37 15 6.16 A3V
HR 3289 22 BD-12 2490 70673 154177 4046 08 22 46.8 -13 03 17 6.11 gG7
HR 3291 CD-25 5988 70761 175709 6782 08 22 49.9 -26 20 53 5.90 F3Ib 0.1 0.1 D:AB, sep 0.100", unresolved by speckle interferometry.
HR 3296 CD-37 4638 70946 199166 4056 08 23 17.2 -38 17 09 6.32 M1III VAR:7.9 - 8.03B.
HR 3308 BD-22 2262 71141 175777 08 24 55.1 -23 09 13 5.68 A2
HR 3315 CD-23 7277 71176 175783 1221 I 6800 A 08 25 03.7 -24 02 46 5.28 K5III+K1III 3.5 41.0 D:B, K1III optical.
HR 3316 BD-20 2522 71196 175792 08 25 19.1 -21 02 45 6.01 F3V
HR 3317 BD-16 2442 71231 154240 08 25 39.4 -17 26 22 6.44 K0
HR 3320 BD-14 2517 71267 154244 2657 08 25 55.6 -14 55 47 5.98 A5m
HR 3322 CD-42 4219 71302 219890 W 08 24 57.2 -42 46 10 5.98 B3V 0.4 0.4
HR 3324 BD-12 2524 71377 154257 I 4085 08 26 41.9 -12 32 04 5.54 K2III v G:Zeta Her group.
HR 3326 CD-41 4119 71459 219910 08 25 51.9 -42 09 12 5.47 B3V G:Member of the local association (Pleiades group).
HR 3327 CD-38 4462 71487 199222 W A NO Pup 08 26 17.6 -39 03 34 6.53 B9V 0.6 8.0 D:Binary with HR 3328.,RV:Probably blended with HR 3328.,S:H/K/m indicate A6/F1V/F2, respectively.,VAR:EA 6.7 - 7.14v, 1.25686d.
HR 3328 CD-38 4462 71488 199224 W B 08 26 18.2 -39 03 37 7.25 A2V: 0.6 8.0 D:Binary with HR 3327.,RV:Probably blended with HR 3327.
HR 3331 CD-28 6048 71523 175851 08 26 50.8 -29 12 55 6.73 B9.5V
HR 3335 BD-20 2538 71581 175870 W VV Pyx 08 27 33.3 -20 50 38 6.56 A2V 1.1 0.3 VAR:E amp. 0.3p, 4.56960d. Equal min. Redder at both minima.

Legend

Key to columns [154]
HR Harvard Revised Number = Bright Star Number
B Bayer designation (greek letter)
F Flamsteed number
DM Durchmusterung Identification (BD = Bonn; CD = Cordoba; CP = Cape Photographic)
HD Henry Draper Catalog Number
SAO SAO Catalog Number
FK5 FK5 star Number
IR I if infrared source
M* Double or multiple-star code. (A = Astrometric binary; D = Duplicity discovered by occultation; I = Innes, Southern Double Star Catalogue (1927); R = Rossiter, Michigan Publ. 9, 1955; S = Duplicity discovered by speckle interferometry; W = Worley (1978) update of the IDS;)
ADS Aitken's Double Star Catalog (ADS) designation
VarID Variable star identification
RA Right Ascension (J2000.0)
Dec Declination (J2000.0)
vMag Visual magnitude
spType Spectral type
dMag Magnitude difference of double, or brightest multiple
Sep Separation of components in Dmag if occultation binary (arcsec)
Remarks Note on Category (C = Colors; D = Double and multiple stars; DYN = Dynamical parallaxes; G = Group membership; M = Miscellaneous; N = Star names; P = Polarization; R = Stellar radii or diameters; RV = Radial and/or rotational velocities; S = Spectra; SB = Spectroscopic binaries; VAR = Variability)

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