فهرست ستاره‌های شاه‌تخته

این صفحه فهرست ستاره‌های صورت فلکی شاه‌تخته است.

نام	B	F	HD	HIP	بعد	میل	vis. mag.	abs. mag.	فاصله (ly)	رده‌بندی	یادداشت
Canopus	α		45348	30438	06 23 57.09	‏44.6″41′‎−52°	−0.72	−5.53	313	F0Ib	Suhel; 2nd brightest star, nearest supergiant
β Car	β		80007	45238	09 13 12.24	‏02.9″43′‎−69°	1.67	−0.99	111	A2IV	Miaplacidus
ε Car	ε		71129	41037	08 22 30.86	‏34.3″30′‎−59°	1.86	−4.58	632	K3III+B2V	Avior; suspected eclipsing binary, V_max = 1.82, V_min = 1.94
ι Car	ι		80404	45556	09 17 05.43	‏30.9″16′‎−59°	2.23	−4.43	692	A8Ib	Aspidiske, Turais, Scutulum; suspected variable, V_max = 2.23, V_min = 2.28
θ Car	θ		93030	52419	10 42 57.43	‏40.1″23′‎−64°	2.74	−2.91	439	B0Vp	in IC 2602
υ Car	υ		85123	48002	09 47 06.14	‏19.3″04′‎−65°	2.92	−5.56	1622	A9	binary star
ω Car	ω		89080	50099	10 13 44.28	‏16.5″02′‎−70°	3.29	−1.99	370	B8III
p Car	p	PP	91465	51576	10 32 01.48	‏07.3″41′‎−61°	3.30	−2.62	497	B4Vne	γ Cas variable, V_max = 3.22, V_min = 3.55
V337 Car	q	V337	89388	50371	10 17 05.01	‏56.4″19′‎−61°	3.39	−3.38	736	K3II	irregular variable, V_max = 3.36, V_min = 3.44
a Car	a	V357	79351	45080	09 10 58.11	‏00.9″58′‎−58°	3.43	−2.11	418	B2IV	eclipsing binary, V_max = 3.41, V_min = 3.44
χ Car	χ		65575	38827	07 56 46.74	‏56.6″58′‎−52°	3.46	−1.91	387	B3IVp	β Cep variable, ΔV = 0.015, P = 0.10 d
l Car	l		84810	47854	09 45 14.83	‏28.5″30′‎−62°	3.69	−4.64	1509	G5Iab/Ib	classical Cepheid, V_max = 3.28, V_min = 4.18, P = 35.54 d
HD 94510	u		94510	53253	10 53 29.57	‏11.8″51′‎−58°	3.78	1.42	97	K0III-IV...	suspected variable, V_max = 3.75, V_min = 3.80
HD 90853	s		90853	51232	10 27 52.75	‏21.9″44′‎−58°	3.81	−3.71	1042	F2II	suspected variable
HD 76728	c		76728	43783	08 55 02.86	‏41.0″38′‎−60°	3.84	−1.06	312	B8III	double star
V382 Car	x	V382	96918	54463	11 08 35.40	‏30.2″58′‎−58°	3.93	−7.37	5927	G0Ia0	hypergiant; slow irregular variable, V_max = 3.77, V_min = 4.05
HD 79447	i		79447	45101	09 11 16.77	‏01.3″19′‎−62°	3.96	−1.97	499	B3IV	variable star, ΔV = 0.008, P = 22.26 d
HD 90589	I		90589	50954	10 24 23.74	‏53.6″01′‎−74°	3.99	2.94	53	F2IV	suspected variable, V_max = 3.96, V_min = 4.00
HD 83183	h		83183	46974	09 34 26.66	‏47.2″13′‎−59°	4.08	−4.83	1976	B5II
V343 Car	d	V343	74375	42568	08 40 37.04	‏39.7″45′‎−59°	4.31	−3.87	1411	B1.5III	β Cep variable
HD 80230	g		80230	45496	09 16 12.10	‏29.2″32′‎−57°	4.34	−1.74	536	M1III	suspected variable, V_max = 4.31, V_min = 4.35
HD 47306	N		47306	31407	06 34 58.59	‏32.3″58′‎−52°	4.35	−4.31	1762	B9III
HR 2554	A	V415	50337	32761	06 49 51.32	‏21.0″37′‎−53°	4.39	−1.74	553	G6II	Algol variable, ΔV = 0.06
HD 91942	r		91942	51849	10 35 35.31	‏27.5″33′‎−57°	4.45	−3.68	1376	K3/K4II	suspected variable
η Car	η		93308		10 45 03.60	‏03.0″41′‎−59°	4.47		7500	LBV	Foramen, Tseen She; in Trumpler 16; binary star; luminous blue variable, V_max = −0.8, V_min = 7.9; surrounded by the Homunculus Nebula; one of the most luminous and most massive stars known.
HR 3643	G		78791	44599	09 05 08.83	‏09.7″36′‎−72°	4.47	−1.25	454	F6II-III
V344 Car	f	V344	75311	43105	08 46 42.56	‏11.3″46′‎−56°	4.50	−1.62	546	B3Vne	γ Cas variable, V_max = 4.40, V_min = 4.51
HD 83944	m		83944	47391	09 39 21.04	‏41.2″19′‎−61°	4.51	0.33	224	B9V	suspected variable
V520 Car	w	V520	93070	52468	10 43 32.31	‏59.9″33′‎−60°	4.58	−2.99	1065	K3Ib	irregular variable, V_max = 4.50, V_min = 4.59
V533 Car	y	V533	97534	54751	11 12 36.02	‏03.5″19′‎−60°	4.59	−8.34	12538	A6Ia	α Cyg variable
HD 96566	z		96566	54301	11 06 32.47	‏26.9″25′‎−62°	4.62	−0.65	370	G8III
V399 Car	P	V399	90772	51192	10 27 24.48	‏19.7″38′‎−57°	4.65			A6Ia	semiregular variable, V_max = 4.63, V_min = 4.72, P = 88.3 d
V345 Car	E	V345	78764	44626	09 05 38.38	‏18.7″32′‎−70°	4.67	−2.94	1079	B2IVe	γ Cas variable, V_max = 4.67, V_min = 4.78, P = 137.7 d
HD 92397	t		92397	52102	10 38 45.01	‏58.8″10′‎−59°	4.69	−4.08	1852	K4/K5III:	suspected variable
HD 91375	K		91375	51438	10 30 20.08	‏33.8″59′‎−71°	4.72	0.22	259	A2III
HR 3220	B		68456	39903	08 09 00.86	‏06.1″18′‎−61°	4.74	3.09	70	F5V
V518 Car		V518	92938	52370	10 42 14.14	‏59.2″27′‎−64°	4.76	−0.97	456	B3V	in IC 2602; γ Cas variable
HD 81101	k		81101	45856	09 20 56.83	‏16.7″24′‎−62°	4.79	0.62	223	G6III
HD 93194			93194	52502	10 44 06.94	‏40.0″57′‎−63°	4.80	−1.06	484	B5Vn	in IC 2602; suspected irregular variable, V_max = 4.79, V_min = 4.84
HD 66591	D		66591	39138	08 00 19.97	‏03.0″34′‎−63°	4.81	−1.29	542	B3V	suspected variable
HD 73389	e		73389	42134	08 35 19.65	‏33.5″00′‎−58°	4.84	0.60	229	K0III
HD 93607			93607	52736	10 46 51.24	‏00.6″23′‎−64°	4.87	−0.83	449	B3IV	in IC 2602; suspected variable
HD 61248	Q		61248	36942	07 35 39.70	‏01.7″32′‎−52°	4.93	−0.48	394	K3III	suspected variable
V376 Car	b	V376	77002	43937	08 56 58.43	‏45.7″13′‎−59°	4.93	−1.47	621	B2IV-V	β Cep variable, V_max = 4.91, V_min = 4.96, P = 0.021 d
HD 91496			91496	51495	10 31 02.07	‏17.4″13′‎−73°	4.94	−2.42	964	K4/K5III	suspected variable, V_max = 4.87, V_min = 4.97
HD 90264	L		90264	50847	10 22 58.18	‏05.5″54′‎−66°	4.97	−0.63	430	B8V
HD 92063	t		92063	51912	10 36 20.56	‏51.5″33′‎−59°	5.08	0.50	269	K1III
HD 59219			59219	36114	07 26 21.86	‏06.6″01′‎−51°	5.09	−1.09	562	K0III
HD 96919	z	V371	96919	54461	11 08 34.01	‏49.8″56′‎−61°	5.12	−6.03	5525	B9Ia	α Cyg variable, V_max = 5.12, V_min = 5.19
HD 53047			53047	33779	07 00 51.51	‏09.5″24′‎−51°	5.14	−1.25	617	M1III	semiregular variable
V386 Car		V386	54118	34105	07 04 18.32	‏59.0″44′‎−56°	5.14	0.45	282	A0p:	α CVn variable, ΔV = 0.026, P = 3.28 d
HD 88981	M		88981	50083	10 13 30.68	‏22.2″22′‎−66°	5.15	0.31	304	Am
HD 69863	C		69863	40429	08 15 15.95	‏56.2″54′‎−62°	5.16	0.81	242	A+...	binary star
HD 77370	b		77370	44143	08 59 24.38	‏03.8″05′‎−59°	5.17	3.08	85	F3V
HR 3153		V460	66342	39070	07 59 37.55	‏13.5″35′‎−60°	5.19	−2.34	1045	M0II	in NGC 2516; semiregular variable, V_max = 5.15, V_min = 5.3
HD 97583			97583	54767	11 12 45.27	‏11.2″10′‎−64°	5.22	0.30	314	B9V	double star
HD 93549			93549	52701	10 46 29.61	‏47.7″15′‎−64°	5.23	−0.37	429	B7IV	in IC 2602
HD 88323			88323	49698	10 08 42.84	‏55.9″48′‎−65°	5.26	0.16	341	K0III	optical double
V524 Car		V524	94367	53154	10 52 30.85	‏25.5″14′‎−57°	5.26	−6.08	6037	B9Ia	α Cyg variable
HD 73390	e		73390	42129	08 35 15.58	‏29.1″13′‎−58°	5.27	−2.08	962	B3V+...
HD 91056			91056	51313	10 28 52.60	‏20.2″10′‎−64°	5.27	−4.64	3135	K3Ib	slow irregular variable
HD 80951			80951	45581	09 17 25.21	‏39.8″53′‎−74°	5.28	−1.44	721	A1V
HD 84121			84121	47479	09 40 42.60	‏00.9″59′‎−57°	5.30	1.16	220	A3IV
HD 93540			93540	52678	10 46 16.58	‏52.5″30′‎−64°	5.33	−0.45	466	B7:V	in IC 2602; suspected variable
HD 92964		V519	92964	52405	10 42 40.57	‏56.8″12′‎−59°	5.36	−6.23	6792	B2.5Ia	α Cyg variable, V_max = 5.32, V_min = 5.43, P = 14.68 d
HD 57917			57917	35589	07 20 38.81	‏09.3″05′‎−52°	5.38	−0.52	493	B9V
HD 80671			80671	45571	09 17 17.40	‏22.5″41′‎−68°	5.38	2.75	109	F4V
HD 49689			49689	32494	06 46 52.69	‏55.6″15′‎−51°	5.39	−1.83	906	K1II/IIIp+G:	suspected variable
HD 73887			73887	42286	08 37 18.85	‏12.3″51′‎−62°	5.45	0.39	335	K0III
HD 82350			82350	46358	09 27 06.50	‏07.5″36′‎−71°	5.46	1.51	201	K2III
HD 83095	H		83095	46741	09 31 36.32	‏51.3″04′‎−73°	5.46	−1.47	791	K4III
HD 92207		V370	92207	52004	10 37 27.08	‏00.0″44′‎−58°	5.47	−6.52	8150	A0Ia	α Cyg variable, V_max = 5.45, V_min = 5.52, P = 1.33 d
V450 Car		V450	53921	34000	07 03 15.11	‏41.3″10′‎−59°	5.50	−0.35	482	B9IV	53 Per variable , ΔV = 0.02
HD 92664		V364	92664	52221	10 40 11.46	‏00.9″06′‎−65°	5.51	−0.26	466	B9p Si	α CVn variable, V_max = 5.48, V_min = 5.52, P = 1.67 d
HD 67364			67364	39566	08 05 03.71	‏28.5″06′‎−53°	5.52	0.11	393	K3/K4III
HD 79698			79698	45219	09 12 55.62	‏50.3″24′‎−59°	5.54	−0.28	475	G6II
HD 85656			85656	48310	09 50 55.60	‏42.5″44′‎−62°	5.56	−1.78	959	K1IIICN...
HD 64067			64067	38152	07 49 06.72	‏37.4″24′‎−56°	5.57	−1.72	934	G5II
HD 46569			46569	31079	06 31 18.22	‏34.3″49′‎−51°	5.58	2.73	121	F8V
HD 96706			96706	54327	11 06 49.93	‏40.6″52′‎−70°	5.58	−2.12	1128	B2V	variable star, ΔV = 0.004, P = 1.74 d
HD 65907			65907	38908	07 57 46.30	‏12.1″18′‎−60°	5.59	4.54	53	G2V...
HD 76113			76113	43499	08 51 36.53	‏01.0″38′‎−57°	5.59	−1.12	716	B8III
V448 Car	O	V448	49877	32531	06 47 18.71	‏24.2″32′‎−55°	5.60	−0.72	598	K5III	semiregular variable
HD 65273			65273	38656	07 54 53.39	‏10.4″18′‎−57°	5.62	0.51	343	K3/K4III
HD 68434			68434	39957	08 09 33.63	‏07.7″05′‎−56°	5.66	0.33	380	A3m...
HD 89715			89715	50520	10 19 05.12	‏34.6″40′‎−64°	5.66	0.90	292	A1V
V372 Car		V372	64722	38438	07 52 29.75	‏01.9″22′‎−54°	5.69	−2.56	1462	B1.5IV	β Cep variable, ΔV = 0.027, P = 0.12 d
HD 88661		QY	88661	49934	10 11 46.47	‏38.0″03′‎−58°	5.70	−2.29	1294	B2IVnpe	γ Cas variable, V_max = 5.63, V_min = 5.83
S Car		S	88366	49751	10 09 22.01	‏57.1″32′‎−61°	5.71		1780	K5-M6e	Mira variable, V_max = 4.5, V_min = 9.9, P = 149.49 d
HD 97670			97670	54829	11 13 30.79	‏09.5″37′‎−59°	5.73	−3.00	1821	B1.5V	suspected variable
HD 65662			65662	38783	07 56 18.65	‏35.3″31′‎−60°	5.74	−2.17	1244	K4II	in NGC 2516
HD 93163			93163	52487	10 43 51.21	‏56.6″14′‎−64°	5.75	−1.71	1009	B3:V	suspected eclipsing binary, ΔV = 0.03
HD 66194		V374	66194	38994	07 58 50.56	‏28.2″49′‎−60°	5.77	−1.72	1028	B2IVnpe	in NGC 2516; γ Cas variable, V_max = 5.72, V_min = 5.84
HD 81830			81830	46225	09 25 27.38	‏02.2″57′‎−61°	5.77	1.47	236	A4V+...
HD 64185			64185	38160	07 49 12.95	‏02.5″17′‎−60°	5.78	3.06	114	F1V	spectroscopic binary
HD 76538			76538	43669	08 53 48.67	‏14.2″21′‎−60°	5.78	−2.35	1376	B5III
HD 85655			85655	48339	09 51 12.03	‏32.4″25′‎−59°	5.79	−1.01	746	K2IIICNp...
HD 77615			77615	44256	09 00 45.75	‏49.8″57′‎−60°	5.80	−2.13	1259	G8II
HD 84152			84152	47498	09 41 02.10	‏34.0″15′‎−57°	5.80	0.57	362	K0/K1III
HD 88473			88473	49764	10 09 30.20	‏58.2″40′‎−68°	5.80	−0.46	583	A0IV
HD 49517			49517	32402	06 45 53.72	‏35.0″24′‎−52°	5.81	−2.32	1376	K3III
HD 93943			93943	52922	10 49 24.46	‏25.6″19′‎−59°	5.85	−1.24	853	B9.5IV/V
HD 80950			80950	45585	09 17 27.63	‏04.8″44′‎−74°	5.86	1.32	264	A0V
HD 60060			60060	36444	07 29 59.74	‏04.6″39′‎−52°	5.87	0.84	330	K0III
HD 66441			66441	39184	08 00 49.96	‏04.7″09′‎−54°	5.87	−0.79	700	B5Vn	suspected variable
V482 Car		V482	82536	46620	09 30 23.45	‏42.9″21′‎−58°	5.88	−1.68	1058	M2III	semiregular variable
V514 Car		V514	92287	52043	10 38 02.66	‏22.7″15′‎−57°	5.89	−2.08	1278	B3IV	rotating ellipsoidal variable, V_max = 5.88, V_min = 5.92, P = 2.90 d
HD 82406			82406	46460	09 28 30.60	‏07.2″42′‎−66°	5.90	1.33	268	A0V
HD 82347			82347	46482	09 28 47.19	‏23.5″16′‎−62°	5.91	0.06	482	K1III
HD 87283			87283	49164	10 02 00.11	‏15.2″25′‎−60°	5.93	−4.03	3196	A9IV	possibly in NGC 3114
HD 90454			90454	50993	10 24 59.50	‏34.7″34′‎−58°	5.93	1.13	297	F2III
T Car		T	94776	53394	10 55 17.26	‏01.9″31′‎−60°	5.93	1.07	306	K0III	not variable
HD 60228			60228	36496	07 30 30.91	‏58.0″23′‎−54°	5.95	0.33	433	M1III
HD 94683			94683	53334	10 54 29.60	‏35.8″49′‎−61°	5.95	−2.59	1663	K4III	suspected variable
HD 54732			54732	34349	07 07 13.30	‏06.2″58′‎−51°	5.96	−0.23	564	K0III
HD 56705			56705	35084	07 15 21.27	‏58.3″29′‎−52°	5.96	0.58	389	K0V
HD 70839			70839	40932	08 21 12.10	‏23.6″58′‎−57°	5.96	−3.36	2380	B1.5III
HD 92436			92436	52127	10 38 59.70	‏00.8″49′‎−58°	5.96	−0.53	648	M1III
HD 91533			91533	51623	10 32 47.82	‏00.3″40′‎−58°	5.98	−6.71	11241	A2Iab	suspected variable
V522 Car		V522	93737	52827	10 48 05.42	‏09.0″55′‎−59°	5.98			A0Ia	α Cyg variable
HD 81613			81613	46101	09 24 05.50	‏55.6″38′‎−61°	5.99	0.92	337	K0III
HD 94650			94650	53272	10 53 42.13	‏13.2″43′‎−70°	5.99	−0.89	776	B6V
HD 98560			98560	55280	11 19 16.84	‏57.4″34′‎−64°	5.99	3.12	122	F6IV
HD 90874			90874	51194	10 27 25.40	‏17.0″42′‎−65°	6.00	1.76	229	A2V
HD 53349			53349	33800	07 01 05.18	‏25.1″56′‎−58°	6.01	2.36	175	F0V	suspected variable
HD 76346			76346	43620	08 53 03.80	‏58.5″38′‎−56°	6.02	1.23	296	A0V	has a planet (b)
HD 80094			80094	45418	09 15 17.66	‏18.2″23′‎−58°	6.02	0.00	522	B7IV	variable star, ΔV = 0.008, P = 1.56 d
HD 56239			56239	34780	07 12 01.98	‏24.2″11′‎−63°	6.03	−0.29	598	A0IV/V
HD 57852			57852	35564	07 20 21.46	‏42.8″18′‎−52°	6.05		113	F5V	component of the HIP 35564 system; suspected variable
HD 82068			82068	46328	09 26 44.18	‏47.5″55′‎−64°	6.05	1.88	223	A3Vn
V390 Car		V390	61966	37248	07 39 00.34	‏24.2″16′‎−53°	6.06	−0.05	544	B9IV-Vp...	α CVn variable, ΔV = 0.004
V535 Car		V535	98292	55140	11 17 19.02	‏24.6″49′‎−67°	6.06	−2.52	1698	M2III	slow irregular variable
HD 88825			88825	50044	10 13 01.16	‏05.1″55′‎−59°	6.07	−2.84	1976	B4Ve
HD 96544			96544	54294	11 06 29.30	‏30.1″40′‎−58°	6.07	−1.81	1226	K2II/III
HD 92682			92682	52150	10 39 15.94	‏36.2″29′‎−74°	6.08	−1.57	1105	K3II	variable star, ΔV = 0.005, P = 0.084 d
HD 63382			63382	37854	07 45 35.52	‏21.3″43′‎−56°	6.10	−1.20	942	F0II
R Car		R	82901	46806	09 32 14.60	‏20.0″47′‎−62°	6.10		416	M6.5 IIIpev	Mira variable, V_max = 3.9, V_min = 10.5, P = 308.71 d
HD 91619		V369	91619	51676	10 33 25.40	‏24.6″11′‎−58°	6.11	−6.99	13583	B7Ia	α Cyg variable, ΔV = 0.1, P = 1.12 d
U Car		U	95109	53589	10 57 48.19	‏55.9″43′‎−59°	6.11			G3Ia	classical Cepheid, V_max = 5.74, V_min = 6.96, P = 38.83 d
HD 70982			70982	40926	08 21 07.65	‏21.4″06′‎−64°	6.11	0.34	464	G6/G8III
V461 Car		V461	66546	39225	08 01 23.05	‏56.0″30′‎−54°	6.12	−1.92	1320	B2IV-V	Algol variable
HD 65908			65908	38863	07 57 12.76	‏48.8″17′‎−63°	6.14	0.37	464	B8V
V478 Car		V478	80710	45615	09 17 51.67	‏03.2″03′‎−67°	6.14	−1.96	1358	K2III	semiregular variable
HD 87543			87543	49281	10 03 34.14	‏02.6″53′‎−61°	6.14	−2.49	1734	B4:Vne
HD 95208			95208	53546	10 57 15.81	‏59.2″05′‎−75°	6.16	−3.12	2345	K1II
HD 95324			95324	53701	10 59 14.05	‏14.7″19′‎−61°	6.16	0.93	363	B8IV
HD 96088			96088	54082	11 04 00.25	‏19.2″57′‎−57°	6.16	−3.63	2964	B3III
HD 47001			47001	31265	06 33 26.31	‏45.5″19′‎−52°	6.18	−0.17	607	G8III
V492 Car		V492	86659	48782	09 56 59.84	‏06.6″06′‎−69°	6.18	−1.43	1087	B3V	53 Per variable
HD 87436			87436	49233	10 02 59.95	‏43.3″10′‎−60°	6.18	−3.80	3228	A6II/III	suspected variable
HD 90630			90630	50976	10 24 44.56	‏18.3″58′‎−73°	6.18	0.53	441	A2/A3V	suspected variable
V655 Car		V655	91272	51425	10 30 08.81	‏04.8″59′‎−66°	6.19	−1.70	1235	B4IV	Algol variable, V_max = 6.19, V_min = 6.36, P = 16.93 d
HD 62897			62897	37599	07 42 53.36	‏48.5″13′‎−58°	6.20	−0.23	629	K0III
HD 75086			75086	42936	08 45 05.55	‏27.6″43′‎−58°	6.20	−1.23	997	B7III
HD 87238			87238	49160	10 01 58.09	‏59.4″20′‎−57°	6.20	−0.62	753	K1II
HD 84850			84850	47913	09 45 55.82	‏38.4″47′‎−58°	6.22	1.68	264	F5IV
HD 89263			89263	50287	10 16 03.26	‏12.4″54′‎−59°	6.22	1.63	270	A5V
V532 Car		V532	97451	54708	11 12 03.60	‏24.1″25′‎−58°	6.24	−0.53	736	M4III	semiregular variable
HD 91767			91767	51732	10 34 12.72	‏15.5″59′‎−60°	6.25	−0.78	830	K2/K3III	suspected variable
HD 65750		V341	65750	38834	07 56 50.70	‏35.0″07′‎−59°	6.25		967	M0III	semiregular variable, V_max = 6.2, V_min = 7.1
HD 93344			93344	52520	10 44 20.10	‏35.0″51′‎−70°	6.25	1.12	346	A5IV/V
HD 52603			52603	33588	06 58 39.81	‏44.1″43′‎−55°	6.26	1.59	280	K2III
HD 74622			74622	42717	08 42 20.90	‏28.8″46′‎−55°	6.26	1.23	331	K2III
υ Car B	υ		85124		09 47 06.70	‏21.0″04′‎−65°	6.26		1623	A8 Ib	component of the υ Car system
HD 93372			93372	52535	10 44 27.25	‏37.1″26′‎−72°	6.26	3.74	104	F6V
HD 93502			93502	52679	10 46 17.12	‏10.4″36′‎−60°	6.26	1.01	365	A0IV
HD 94491			94491	53231	10 53 21.18	‏36.5″53′‎−58°	6.26	−2.16	1575	B5V
HD 82858			82858	46737	09 31 33.05	‏08.6″43′‎−66°	6.27	−0.40	703	K1III
HD 66607			66607	39238	08 01 31.58	‏16.8″27′‎−55°	6.28	−0.28	668	B4V
V375 Car		V375	67536	39530	08 04 42.94	‏10.9″50′‎−62°	6.29		1249	B2.5Vn	β Cep variable, ΔV = 0.04, P = 1.02 d
HD 61031			61031	36856	07 34 39.58	‏28.3″28′‎−51°	6.29	−1.76	1331	A1III/IV
HD 93662			93662	52797	10 47 38.41	‏02.7″28′‎−57°	6.29	−3.35	2763	M1II	suspected variable, V_max = 6.28, V_min = 6.41
HD 94275			94275	53100	10 51 46.93	‏20.3″16′‎−57°	6.29	−0.05	604	A6III
HD 63926			63926	38087	07 48 19.51	‏15.9″28′‎−56°	6.30	−2.91	2264	K0III+...
HD 66341			66341	39073	07 59 40.09	‏26.6″12′‎−60°	6.30	−1.81	1364	B8III	in NGC 2516
HD 81502			81502	46049	09 23 27.33	‏08.4″18′‎−60°	6.30	−2.91	2264	K1/K2II/III
HD 86606			86606	48715	09 56 09.76	‏21.5″23′‎−71°	6.30	−2.69	2050	B1Ib
HD 68423			68423	39843	08 08 24.65	‏03.0″48′‎−63°	6.32	−0.58	782	B6V	suspected variable
HD 80126			80126	45437	09 15 34.73	‏39.9″34′‎−57°	6.32	−1.32	1098	G8II
QZ Car		QZ	93206	52526	10 44 22.92	‏36.0″59′‎−59°	6.32	−3.23	2650	B0Ib:	in Collinder 228; β Lyr variable, V_max = 6.16, V_min = 6.49, P = 6.00 d
HD 82458			82458	46407	09 27 49.19	‏52.3″46′‎−71°	6.33	2.57	184	F3/F5V
V486 Car		V486	84416	47591	09 42 12.99	‏53.4″54′‎−66°	6.33	0.04	592	A0V	β Lyr variable
HD 92536			92536	52160	10 39 22.85	‏42.5″06′‎−64°	6.33	0.49	479	B8V	in IC 2602
HD 74341			74341	42579	08 40 43.55	‏43.9″32′‎−57°	6.34	2.13	227	A3V
HD 90074			90074	50785	10 22 10.48	‏56.3″15′‎−58°	6.34	1.23	343	G6III
HD 90289			90289	50916	10 23 50.66	‏14.1″57′‎−57°	6.34	−0.59	793	K5Ib-II	suspected variable, V_max = 6.33, V_min = 6.35
HD 93649			93649	52730	10 46 48.09	‏35.3″12′‎−69°	6.34	−2.04	1545	A2IV
HD 97472			97472	54673	11 11 29.57	‏10.3″26′‎−71°	6.34	0.08	583	K2/K3III
HD 74148			74148	42440	08 39 13.24	‏02.4″19′‎−60°	6.35	0.71	437	A0V
HD 89805			89805	50562	10 19 42.04	‏14.1″08′‎−65°	6.35	−2.59	2000	K2II
WR 22		V429	92740	52308	10 41 17.52	‏36.9″40′‎−59°	6.35	−4.72	5344	WN7 + A(SB1)	Wolf–Rayet star and Algol variable, V_max = 6.33, V_min = 6.52, P = 80.34 d; one of the most luminous stars known
HD 93739			93739	52785	10 47 30.62	‏15.8″26′‎−69°	6.35	−1.57	1249	B2IV
HD 65189			65189	38667	07 55 00.44	‏00.1″35′‎−52°	6.36	−1.08	1003	B8III
HD 72322			72322	41653	08 29 36.40	‏27.3″11′‎−55°	6.36	−0.36	721	G0V
V473 Car		V473	76640	43763	08 54 54.05	‏22.9″14′‎−58°	6.36	−0.77	869	B5V	53 Per variable
HD 79699			79699	45214	09 12 50.63	‏00.5″55′‎−60°	6.36	0.21	553	B9V
HD 78632			78632	44665	09 06 07.61	‏59.7″29′‎−64°	6.37	0.08	590	K3III
HD 61394			61394	36977	07 36 01.62	‏15.8″53′‎−55°	6.39	0.06	601	K1/K2IIICN.
HD 96568			96568	54289	11 06 24.32	‏23.8″50′‎−64°	6.39	0.58	473	A3V
HD 44267			44267	29913	06 17 51.74	‏58.9″43′‎−52°	6.40	−0.70	858	K2/K3III	variable star, ΔV = 0.008, P = 1.32 d
HD 62758			62758	37530	07 42 10.22	‏51.4″37′‎−58°	6.40	−1.18	1069	B2.5V
V368 Car		V368	88647	49926	10 11 35.49	‏40.2″49′‎−58°	6.40		801	M3III	semiregular variable, V_max = 6.1, V_min = 6.4
HD 51210			51210	33012	06 52 45.44	‏28.6″20′‎−59°	6.41	0.62	470	A3m...
HD 87438			87438	49223	10 02 49.42	‏24.0″09′‎−62°	6.41	−3.23	2763	K3Ib	irregular variable, V_max = 6.38, V_min = 6.43
HD 91270			91270	51461	10 30 39.24	‏23.4″21′‎−61°	6.41	−0.57	811	M2III	suspected variable
HD 84046			84046	47422	09 39 45.15	‏34.7″56′‎−62°	6.42	0.01	623	B8/B9III/IVw...	suspected variable, V_max = 6.42, V_min = 6.8
HD 88907			88907	50067	10 13 21.20	‏31.8″39′‎−61°	6.42	−1.06	1022	B2V
V507 Car		V507	90966	51265	10 28 18.28	‏52.5″09′‎−63°	6.42	−2.56	2037	B2/B3III:ne	Be star
HD 91094			91094	51327	10 29 03.67	‏34.8″10′‎−65°	6.42	0.00	627	M1III	semiregular variable
HD 98025			98025	55003	11 15 42.76	‏21.1″21′‎−57°	6.42	0.16	583	A3V
HD 78293			78293	44565	09 04 48.00	‏09.5″51′‎−57°	6.43	−1.21	1101	A8III
HD 93359			93359	52537	10 44 32.42	‏18.9″51′‎−70°	6.43	1.25	354	A6IV
HD 65867			65867	38963	07 58 21.47	‏54.9″26′‎−51°	6.44	0.43	518	A8/A9IV	suspected eclipsing binary
V469 Car		V469	72303	41644	08 29 29.82	‏42.5″12′‎−54°	6.44	−0.28	720	Ap Si	α CVn variable
HD 49705			49705	32477	06 46 41.70	‏42.2″41′‎−54°	6.45	0.93	414	G6III
HD 81896			81896	46143	09 24 37.16	‏32.8″04′‎−70°	6.45	0.06	617	K1III
V495 Car		V495	88158	49642	10 07 56.64	‏17.2″13′‎−62°	6.45	−0.55	817	Ap Si	α CVn variable
WR 24			93131	52488	10 43 52.27	‏04.0″07′‎−60°	6.46	−5.05	6520	WN7 + A	in Collinder 228; Wolf–Rayet star, V_max = 6.46, V_min = 6.49, P = 4.76 d; one of the most luminous stars known
HD 52622			52622	33577	06 58 36.39	‏41.2″23′‎−56°	6.46	1.46	326	F2II	suspected variable
HD 54967			54967	34350	07 07 16.28	‏59.2″42′‎−59°	6.46	−1.79	1455	B3V
HD 93738			93738	52815	10 47 53.55	‏46.3″15′‎−64°	6.46	0.67	469	B9.5V	in IC 2602
HD 49219			49219	32269	06 44 12.81	‏43.9″41′‎−54°	6.47	−0.30	736	B5/B6V	variable star, ΔV = 0.011, P = 1.60 d
HD 70267			70267	40655	08 17 55.79	‏00.3″10′‎−59°	6.47	2.01	254	F5V
V487 Car		V487	84809	47893	09 45 40.64	‏09.8″11′‎−57°	6.47	−0.66	869	B8III/IV	α CVn variable
HD 93695			93695	52806	10 47 44.34	‏30.9″52′‎−59°	6.47	−1.41	1230	B5Vvar
HD 95122			95122	53556	10 57 20.22	‏17.0″02′‎−69°	6.48	−0.55	832	B7V	suspected variable
HD 92399			92399	52103	10 38 45.39	‏44.7″15′‎−59°	6.50	−1.82	1502	B4/B5III/IV
HD 96248		V414	96248	54179	11 04 57.57	‏32.0″51′‎−59°	6.58		3700	B1Iab	α Cyg variable, V_max = 6.53, V_min = 6.62, P = 8.52 d
HD 57853			57853	35564	07 20 21.43	‏31.91″18′‎−52°	6.63		113	F9V	component of the HIP 35564 system
QX Car		QX	86118	48589	09 54 33.88	‏16.6″25′‎−58°	6.64		1610	B2V	Algol variable, V_max = 6.6, V_min = 7.21, P = 4.48 d
HD 96446		V430	96446	54266	11 06 05.82	‏59.6″56′‎−59°	6.68		1540	B2k	β Cep variable, ΔV = 0.03
HD 53143			53143	33690	06 59 59.66	‏10.3″20′‎−61°	6.68		59.74	G9V	has a circumstellar disk
VY Car		VY	93203	52538	10 44 32.69	‏55.3″33′‎−57°	6.91		9100	F7Iab/Ib	classical Cepheid, V_max = 6.91, V_min = 8.00, P = 18.89 d
AG Car		AG	94910	53461	10 56 11.58	‏12.8″27′‎−60°	6.96		17000	B2-3Ib/WN11	luminous blue variable, V_max = 5.7, V_min = 8.3, P = 371.4 d
BO Car		BO	93420		10 45 50.63	‏19.5″29′‎−59°	7.18			M4Iab:	semiregular variable, V_max = 7.15, V_min = 7.95, P = 130.7 d
HD 93403			93403	52628	10 45 44.12	‏28.1″24′‎−59°	7.30		2670	O5.5I+O7V	binary star
HD 93129A			93129A		10 43 57.46	‏51.2″32′‎−59°	7.31		7500	O2If*+O3.5	in Trumpler 14; binary star; primary is one of the most luminous stars known
V Car		V	72275	41588	08 28 43.70	‏21.3″07′‎−60°	7.31		5600	G2Iab:	classical Cepheid, V_max = 7.08, V_min = 7.82, P = 6.70 d
HD 93843			93843		10 48 37.78	‏25.5″13′‎−60°	7.33			O5III(f)v	irregular variable, V_max = 7.31, V_min = 7.35
HD 95086			95086	53524	10 57 03.0	‏02″40′‎−68°	7.36		295	A8III	has a planet (b)
HD 93250			93250	52558	10 44 45.03	‏54.7″33′‎−59°	7.50		7500	O4IIIfc	in Trumpler 16; suspected variable
HR Car		HR	90177	50843	10 22 53.84	‏28.4″37′‎−59°	7.57		17700	B3Iaep	luminous blue variable, V_max = 6.8, V_min = 8.80
WR 40		V385	96548	54283	11 06 17.20	‏35.2″30′‎−65°	7.70		5900	WN8h	Wolf–Rayet star and rotating ellipsoidal variable, ΔV = 0.04, P = 4.76 d; one of the most luminous stars known
HD 93205		V560	93205		10 44 33.74	‏15.5″44′‎−59°	7.75		7500	O3.5V((f+))	in Trumpler 16; rotating ellipsoidal variable, V_max = 7.74, V_min = 7.76, P = 6.08 d
IW Car		IW	82084 82085		09 26 53.30	‏48.9″37′‎−63°	7.90			A4Iab/II:	RV Tau variable, V_max = 7.77, V_min = 9.10, P = 143.6 d
HD 65216			65216	38558	07 53 41.3	‏50.4″38′‎−63°	7.98		112	G5V	has two planets (b & c)
HD 97152		V431	97152	54574	11 10 04.08	‏45.0″58′‎−60°	8.07		4000	WC7+O7V	Wolf–Rayet star; eclipsing binary, V_max = 7.97, V_min = 8.08, P = 1.62 d
HD 63765			63765	38041	07 47 49.72	‏50.9″15′‎−54°	8.10	5.53	106	G9V	Tapecue; has a planet (b)
Y Car		Y	91565	51653	10 33 10.85	‏55.1″29′‎−58°	8.16		3050	F2	double-mode Cepheid, V_max = 7.53, V_min = 8.48, P = 3.64 d
HD 51608			51608	33229	06 54 51	‏34″15′‎−55°	8.17		114	K0IV	has two planets (b & c)
HD 85628 A			85628		09 50 19.2	‏50″06′‎−66°	8.19		559	A3V	has a planet (b)
YZ Car		YZ	90912	51262	10 28 16.85	‏00.7″21′‎−59°	8.24		5900	G5	classical Cepheid, V_max = 8.24, V_min = 9.08, P = 18.17 d
WR 16		V396	86161	48617	09 54 52.90	‏38.3″43′‎−57°	8.32			WN8h	rotating ellipsoidal variable, ΔV = 0.06; one of the most luminous stars known
EM Car		EM	97484		11 12 04.51	‏42.9″05′‎−61°	8.52			O8V	Algol variable
RT Car		RT	303310	52562	10 44 47.15	‏48.1″24′‎−59°	8.55		1430	M2Iab:	possibly in Trumpler 15; irregular variable, V_max = 8.2, V_min = 9.9, one of the largest stars known
HD 85567		V596	85567	48269	09 50 28.54	‏03.0″58′‎−60°	8.57		6900	B2	FS CMa variable, V_max = 8.44, V_min = 8.75
UX Car		UX	91039	51338	10 29 11.24	‏48.3″36′‎−57°	8.62		2530	F2II	classical Cepheid, V_max = 7.81, V_min = 8.67, P = 3.68 d
XZ Car		XZ	305996	54101	11 04 13.47	‏47.7″58′‎−60°	8.67			B2:pe	classical Cepheid, V_max = 8.05, V_min = 9.12, P = 16.65 d
GG Car		GG	94878	53444	10 55 58.92	‏33.4″23′‎−60°	8.70			B0/2eq	Be star and re-radiating binary system, V_max = 8.44, V_min = 9.08, P = 31.03 d
V403 Car		V403			10 35 40.67	‏44.6″12′‎−58°	8.74		8400	B1III	in NGC 3293; β Cep variable, ΔV = 0.033, P = 0.25 d
Tr 16-104		V572			10 44 47.31	‏53.2″43′‎−59°	8.75		7500	O7V((f))+ O9.5V+ B0.2IV	in Trumpler 16; Algol variable, V_max = 8.66, V_min = 9.07, P = 2.15 d
V348 Car		V348	90707		10 29 59.00	‏32.8″40′‎−57°	8.78			B1III	β Lyr variable, V_max = 8.55, V_min = 8.93, P = 5.56 d
WR 25		V396	93162		10 44 10.34	‏11.4″43′‎−59°	8.80		7500	O2.5If*/WN6	in Trumpler 16; Wolf–Rayet star; one of the most luminous stars known
HD 60435		V409	60435	36537	07 30 56.99	‏28.2″59′‎−57°	8.89		739	Ap...	rapidly oscillating Ap star
WR 23			92809	52331	10 41 38.32	‏18.7″46′‎−58°	9.03		3400	WC6	Wolf–Rayet star
HD 92024		V381	92024		10 36 08.31	‏04.77″13′‎−58°	9.04		8400	B1III	in NGC 3293; β Cep variable, V_max = 9.04, V_min = 9.06, P = 0.17 d
GH Car		GH	306077	54621	11 10 44.59	‏01.0″45′‎−60°	9.20			G0	classical Cepheid, V_max = 9, V_min = 9.35, P = 5.73 d
WZ Car		WZ	94777	53397	10 55 18.73	‏24.0″56′‎−60°	9.37		4700	F8	classical Cepheid, V_max = 8.63, V_min = 9.88, P = 23.02 d
CPD -59° 2635		V731			10 45 12.72	‏46.2″44′‎−59°	9.43		7500	O8V+O9.5V	in Trumpler 16; Algol variable, V_max = 9.27, V_min = 9.78, P = 2.30 d
V392 Car		V392			07 58 10.47	‏57.5″51′‎−60°	9.49			A2Vp...	in NGC 2516; Algol and α CVn variable, V_max = 9.49, V_min = 9.67
XY Car		XY	308149	53945	11 02 16.07	‏46.5″15′‎−64°	9.49			G5	classical Cepheid, V_max = 8.82, V_min = 9.77, P = 12.43 d
HD 87643		V640	87643		10 04 30.29	‏52.1″39′‎−58°	9.50			B2e	Orion variable, V_max = 7.4, V_min = 9.8
CPD -59 2628		V573			10 45 08.23	‏49.5″40′‎−59°	9.52		7500	O9.5V+B0.3V	in Trumpler 16; Algol variable
HD 90657		V398	90657	51109	10 26 31.41	‏26.2″38′‎−58°	9.69		3500	WN5+O4-6	Wolf–Rayet star; eclipsing binary, ΔV = 0.035
GL Car		GL	306168		11 14 39.84	‏36.3″39′‎−60°	9.70			B3:V	Algol variable
DW Car		DW	305543		10 43 10.07	‏11.7″02′‎−60°	9.85			B2:pe	in Collinder 228; Algol variable
SS73 17		V648			10 11 02.95	‏13.9″48′‎−57°	9.99			M3pe+OB	Z And variable , V_max = 9.6, V_min = 10.0, P = 520 d
CPD -57 2874					10 15 21.97	‏42.7″51′‎−57°	10.16			sgB1[e]	B[e] star
GZ Car		GZ	302719	50615	10 20 20.37	‏35.8″22′‎−59°	10.20		2400	G5	double-mode Cepheid, V_max = 9.98, V_min = 10.47, P = 4.16 d
HH Car		HH	303503		10 53 36.47	‏18.2″27′‎−59°	10.31			B	Algol variable, V_max = 10.3, V_min = 10.82, P = 3.23 d
EY Car		EY		52380	10 42 23.03	‏57.3″09′‎−61°	10.35			B2:pe	double-mode Cepheid, V_max = 10.01, V_min = 10.56, P = 2.88 d
HD 307938		V557	307938		10 42 41.52	‏04.4″21′‎−64°	10.57			G2V	BY Dra variable, ΔV = 0.21
WR 18		V500	89358	50368	10 17 02.27	‏47.9″54′‎−57°	10.6		6300	WN4-s	Wolf–Rayet star
HD 94546		V428	94546	53274	10 53 44.82	‏46.7″30′‎−59°	10.7			WN4+O8V	Wolf–Rayet star; eclipsing binary, ΔV = 0.05
He 3-519					10 53 59.59	‏44.3″26′‎−60°	10.85			WN11	Wolf–Rayet star, V_max = 10.6, V_min = 11.0
NGC 3603-A1			97950A		11 15 07.31	‏38.4″15′‎−61°	11.12		20000	WN6ha+O3V	in NGC 3603; Algol variable, ΔV = 0.45, P = 3.77 d both components among the most luminous and massive stars known
CR Car		CR			10 32 54.07	‏15.5″31′‎−58°	11.30			B2:pe	classical Cepheid, V_max = 11.3, V_min = 11.89, P = 9.76 d
NGC 3603-B			97950B		11 15 07.41	‏38.6″15′‎−61°	11.33			WN6h+abs	one of the most luminous and most massive stars known
Innes' star					11 16 00.21	‏51.6″32′‎−57°	11.52		41.31	M3.5	has a planet
QU Car		QU	310376	54226	11 05 42.49	‏58.2″37′‎−68°	11.54		1290	B+...	V Sge variable , V_max = 10.9, V_min = 11.7, P = 0.45 d
WR 30		V541	94305		10 51 06.01	‏01.7″17′‎−62°	11.73			WC6+O7.5V	Algol variable, ΔV = 0.09
WRA 751		V432			11 08 40.06	‏51.7″42′‎−60°	11.79			WR:	luminous blue variable, V_max = 10.7, V_min = 12.43
NGC 3603-C			97950C		11 15 07.59	‏18.0″15′‎−61°	11.89			WN6h+abs	spectroscopic binary
FO 15		V662			10 45 36.32	‏23.2″48′‎−59°	12.09		7500	O5.5V+O9.5V	in Trumpler 16; Algol variable, V_max = 12.09, V_min = 12.7, P = 1.41 d
Sher 25					11 15 07.8	‏17″15′‎−61°	12.27			B1.5Iab	in NGC 3603; potential supernova progenitor
WR 30a		V574			10 51 38.93	‏35.2″56′‎−60°	12.73			WR+...	Algol variable, ΔV = 0.05
GJ 1128					09 42 46.356	‏06.04″53′‎−68°	12.78			M4.0V
He 2-38		V366			09 54 43.29	‏52.4″18′‎−57°	12.92			M5-7.5	Mira and Z And variable, V_max = 12.1, V_min = 14.4, P = 433 d
BPM 6502		V727			10 44 10.23	‏18.0″18′‎−69°	13.09			DA2.2+M	re-radiating binary system
WR 20a		V712			10 23 58.00	‏49.0″45′‎−57°	13.5			O3If/WN6+ O3If/WN6	in Westerlund 2; Algol variable
LHS 288					10 44 21.32	‏38.4″12′‎−61°	13.92		15.602	M4
OGLE-TR-113		V752			10 52 24.4	‏48.5″26′‎−61°	14.42		1800	K	has a transiting planet (b)
2S 0921-630		V395			09 22 35.20	‏38.5″17′‎−63°	15.3			K0IIIe	low-mass X-ray binary
OGLE-TR-123		V816			11 06 51.1	‏10.5″11′‎−61°	15.47			FV+MV	possibly has a transiting planet
OGLE-TR-111		V759			10 53 17.9	‏20.3″24′‎−61°	15.55		5000	G	has a transiting planet (b) and a possible second planet
OGLE-TR-132		V742			10 50 34.7	‏25.9″57′‎−61°	15.72		7110	F	has a transiting planet (b)
OY Car		OY			10 06 22.07	‏04.6″14′‎−70°	16.2		277	M5/M6:...	SU UMa variable and eclipsing binary, V_max = 11.2, V_min = 16.2, P = 0.063 d
OGLE-TR-182					11 09 18.73	‏42.93″05′‎−61°	16.84		12700	G	has a transiting planet (b)
OGLE-TR-211					10 40 14.39	‏20.2″27′‎−62°			5300	F	has a transiting planet (b)
OGLE-TR-122		V817			11 06 52.0	‏45.7″51′‎−60°					has a transiting brown dwarf
OGLE2-TR-L9					11 07 55	‏46″08′‎−61°			2935	F3	has a transiting planet (b)
1E 1048.1-5937					10 50 08.93	‏19.9″53′‎−59°				Be	anomalous X-ray pulsar
DENIS J081730.0-615520					08 17 30.01	‏15.8″55′‎−61°			16.1	T6	brown dwarf
PSR J1048-5832					10 48 12.20	‏05.8″32′‎−58°					pulsar
PSR J1119-6127					11 19 14.30	‏49.5″27′‎−61°					pulsar

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فهرست ستارگان بر پایه صورت فلکی

منابع

↑ Kunitzsch, P., & Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 25. ISBN 978-1-931559-44-7.

ویکی‌پدیای انگلیسی

[1] Kunitzsch, P., & Smart, T. (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, MA: Sky Pub. p. 25. ISBN 978-1-931559-44-7.