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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.

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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)

Kataloge

Puppis / Yale Bright Star Catalog (HR)

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