List of stars in Monoceros

This is the list of notable stars in the constellation Monoceros, sorted by decreasing brightness.

More information Name, B ...

Name	B	F	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
Î± Mon	Î±	26		61935	37447	07^h 41^m 14.88^s	â09Â° 33â² 03.9â³	3.94	0.71	144	K0III
Î³ Mon	Î³	5		43232	29651	06^h 14^m 51.34^s	â06Â° 16â² 29.0â³	3.99	â2.49	644	K3III
Î´ Mon	Î´	22		55185	34769	07^h 11^m 51.86^s	â00Â° 29â² 34.0â³	4.15	â1.15	375	A2V
Î¶ Mon	Î¶	29		67594	39863	08^h 08^m 35.66^s	â02Â° 59â² 01.6â³	4.36	â4.41	1852	G2Ib
Îµ Mon A	Îµ	8		44769	30419	06^h 23^m 46.10^s	+04Â° 35â² 34.2â³	4.39	1.41	128	A5IV	component of the Îµ Mon system
13 Mon		13		46300	31216	06^h 32^m 54.23^s	+07Â° 19â² 58.7â³	4.47	â3.86	1509	A0Ib	suspected variable
18 Mon		18		49293	32578	06^h 47^m 51.66^s	+02Â° 24â² 43.9â³	4.48	â0.81	373	K0III
Î² Mon A	Î²	11		45725	30867	06^h 28^m 49.07^s	â07Â° 01â² 59.0â³	4.60	â2.03	691	B3Ve	Herschel's Wonder Star; component of the Î² Mon system; Be star
S Mon		15	S	47839	31978	06^h 40^m 58.66^s	+09Â° 53â² 44.7â³	4.66	â2.82	1022	O7V + O9.5V	in NGC 2264; irregular variable, V_max = 4.62^m, V_min = 4.68^m
28 Mon		28	V645	65953	39211	08^h 01^m 13.30^s	â01Â° 23â² 32.7â³	4.68	â1.12	472	K4III	FK Com variable, ÎV = 0.02^m, P = 0.21 d
17 Mon		17		49161	32533	06^h 47^m 19.84^s	+08Â° 02â² 14.2â³	4.77	â1.09	484	K4III
20 Mon		20		54810	34622	07^h 10^m 13.68^s	â04Â° 14â² 15.5â³	4.91	0.85	211	K0III
3 Mon		3		40967	28574	06^h 01^m 50.43^s	â10Â° 35â² 52.6â³	4.92	â2.47	979	B5III	suspected variable
27 Mon		27		65695	39079	07^h 59^m 44.18^s	â03Â° 40â² 46.5â³	4.93	0.51	250	K2III
19 Mon		19	V637	52918	33971	07^h 02^m 54.78^s	â04Â° 14â² 21.3â³	4.99	â2.68	1116	B1V	Î² Cep variable, V_max = 4.96^m, V_min = 5.01^m, P = 0.19 d
2 Mon		2		40536	28325	05^h 59^m 04.31^s	â09Â° 33â² 29.3â³	5.04	0.02	328	A6m
HD 42690				42690	29417	06^h 11^m 51.82^s	â06Â° 33â² 01.0â³	5.06	â2.78	1203	B2V
10 Mon		10		45546	30772	06^h 27^m 57.57^s	â04Â° 45â² 43.7â³	5.06	â3.03	1353	B2V
HD 49331				49331	32558	06^h 47^m 37.22^s	â08Â° 59â² 54.6â³	5.08	â2.94	1309	M1II	suspected variable, V_max = 5.00^m, V_min = 5.11^m
HD 46487				46487	31278	06^h 33^m 37.92^s	â01Â° 13â² 12.4â³	5.09	â0.99	536	B5Vn
25 Mon		25		61064	37088	07^h 37^m 16.73^s	â04Â° 06â² 39.7â³	5.13	1.18	202	F6III	suspected Î´ Sct variable, ÎV = 0.01^m
HR 2142			V696	41335	28744	06^h 04^m 13.50^s	â06Â° 42â² 32.2â³	5.19	â2.06	918	B2Vne+	unique variable
77 Ori		(77)		45416	30717	06^h 27^m 13.76^s	+00Â° 17â² 57.4â³	5.19	â2.13	950	K1II
HD 48217				48217	32064	06^h 41^m 56.37^s	â09Â° 10â² 02.7â³	5.21	â0.11	378	M0III
HD 52666				52666	33878	07^h 01^m 56.39^s	â05Â° 43â² 19.5â³	5.21	â1.38	682	M2III	suspected variable, V_max = 5.15^m, V_min = 5.21^m
HD 46089				46089	31119	06^h 31^m 48.29^s	+11Â° 32â² 39.6â³	5.22	1.16	211	A3V
7 Mon		7		44112	30073	06^h 19^m 42.80^s	â07Â° 49â² 22.5â³	5.27	â1.74	823	B2.5V
HD 43993				43993	29996	06^h 18^m 50.58^s	â09Â° 23â² 23.9â³	5.36	â0.62	511	K1III
HD 41692				41692	28949	06^h 06^m 38.74^s	â04Â° 11â² 37.8â³	5.37	â3.71	2131	B5IV
Î² Mon B	Î²	11		45726		06^h 28^m 49.50^s	â07Â° 02â² 04.0â³	5.40				Herschel's Wonder Star; component of the Î² Mon system
HD 46229				46229	31121	06^h 31^m 50.07^s	â08Â° 09â² 29.5â³	5.43	â1.70	869	K2III
21 Mon		21	V571	55057	34724	07^h 11^m 23.63^s	â00Â° 18â² 06.9â³	5.44	0.92	261	F2V	Î´ Sct variable, V_max = 5.43^m, V_min = 5.5^m, P = 0.089 d
HD 50747				50747	33184	06^h 54^m 24.66^s	â01Â° 07â² 37.1â³	5.45	â0.42	484	A4IV	Î³ Dor variable, ÎV = 0.001^m, P = 0.21 d
HD 62902				62902	37901	07^h 46^m 02.16^s	â06Â° 46â² 20.2â³	5.49	1.17	238	K5III
HD 47054				47054	31583	06^h 36^m 35.33^s	â05Â° 12â² 40.0â³	5.52	â1.52	834	B8V
78 Ori		(78)		45433	30720	06^h 27^m 15.59^s	â00Â° 16â² 33.6â³	5.55	â1.26	749	K5III
HD 45415				45415	30728	06^h 27^m 20.48^s	+02Â° 54â² 29.7â³	5.55	0.79	292	G9III
Î² Mon C	Î²			45727		06^h 28^m 49.50^s	â07Â° 02â² 04.0â³	5.60				Herschel's Wonder Star; component of the Î² Mon system
HD 46304				46304	31167	06^h 32^m 23.13^s	â05Â° 52â² 07.4â³	5.60	2.42	141	F0Vnn+...
HD 59311				59311	36388	07^h 29^m 18.68^s	â01Â° 54â² 19.1â³	5.60	â2.89	1630	K5III
HD 63752				63752	38253	07^h 50^m 10.58^s	â09Â° 11â² 00.4â³	5.60	â2.57	1405	K3III
HD 53208				53208	34086	07^h 04^m 05.25^s	â05Â° 19â² 26.3â³	5.63	â2.38	1304	K3III	suspected variable
HD 49147				49147	32474	06^h 46^m 39.02^s	â10Â° 06â² 26.5â³	5.66	â0.42	535	B9.5V
HD 49434				49434	32617	06^h 48^m 19.09^s	â01Â° 19â² 07.8â³	5.75	2.74	131	F1V	Î´ Sct and Î³ Dor variable
HD 49643				49643	32698	06^h 49^m 16.41^s	â02Â° 16â² 19.3â³	5.75	â0.42	558	B8IIIn
HD 50277				50277	33024	06^h 52^m 49.49^s	+08Â° 22â² 49.6â³	5.75	1.77	204	F0Vn
HD 59381				59381	36396	07^h 29^m 22.11^s	â10Â° 19â² 36.0â³	5.75	â1.52	926	K5III	slow irregular variable, V_max = 5.74^m, V_min = 5.76^m
HD 64235				64235	38474	07^h 52^m 47.87^s	â05Â° 25â² 41.5â³	5.76	2.70	133	F5IVs	suspected variable, V_max = 5.74^m, V_min = 5.77^m
HD 46769				46769	31446	06^h 35^m 15.83^s	+00Â° 53â² 24.8â³	5.78	â3.94	2860	B8Ib
HD 49933				49933	32851	06^h 50^m 49.82^s	â00Â° 32â² 25.5â³	5.78	3.40	97	F2V
HD 53510				53510	34215	07^h 05^m 39.00^s	+09Â° 11â² 09.0â³	5.78	â0.40	562	M0III	variable star, ÎV = 0.007^m, P = 0.088 d
HD 47964				47964	31992	06^h 41^m 05.45^s	+00Â° 29â² 43.2â³	5.79	â1.96	1156	B8III
HD 55775				55775	34975	07^h 14^m 10.87^s	â03Â° 54â² 06.3â³	5.80	â0.57	613	K5III
U Mon			U	59693	36521	07^h 30^m 47.47^s	â09Â° 46â² 36.8â³	5.82		2248	K0Ibpvar	RV Tau variable, V_max = 5.45^m, V_min = 7.67^m, P = 91.32 d
HD 43157				43157	29629	06^h 14^m 36.71^s	â04Â° 34â² 06.5â³	5.83	â0.56	617	B5V
HD 57749				57749	35749	07^h 22^m 25.40^s	â05Â° 58â² 58.1â³	5.83	â1.39	908	F3IV	suspected Î´ Sct variable, V_max = 5.80^m, V_min = 5.84^m
HD 59380				59380	36399	07^h 29^m 25.61^s	â07Â° 33â² 05.3â³	5.86	3.64	91	F8V
HD 45320				45320	30666	06^h 26^m 39.59^s	â01Â° 30â² 26.2â³	5.87	1.64	229	A3Vn
12 Mon		12		46241	31159	06^h 32^m 19.23^s	+04Â° 51â² 21.6â³	5.87	â0.12	517	K0V	suspected variable, V_max = 5.83^m, V_min = 5.87^m
HD 41547				41547	28854	06^h 05^m 27.02^s	â10Â° 14â² 33.6â³	5.88	2.03	192	F4V:	Î³ Dor variable
HD 45067				45067	30545	06^h 25^m 16.41^s	â00Â° 56â² 43.3â³	5.88	3.28	108	F8V
HD 48434				48434	32226	06^h 43^m 38.65^s	+03Â° 55â² 57.1â³	5.88		2850	B0III	suspected Î² Cep variable
HD 51104				51104	33372	06^h 56^m 25.84^s	+09Â° 57â² 23.8â³	5.90	â0.28	561	B8Vn
HD 55832				55832	34982	07^h 14^m 15.52^s	â09Â° 56â² 51.1â³	5.90	â3.38	2345	K3III
HD 59984				59984	36640	07^h 32^m 05.82^s	â08Â° 52â² 51.3â³	5.90	3.52	98	F5V	suspected variable, V_max = 5.5^m, V_min = 6.8^m
HD 45976				45976	30986	06^h 30^m 11.28^s	â10Â° 04â² 53.4â³	5.92	â5.50	6269	K0
16 Mon		16		48977	32463	06^h 46^m 32.42^s	+08Â° 35â² 13.8â³	5.92	â1.75	1116	B2.5V	53 Per variable, ÎV = 0.01^m, P = 1.94 d
HD 46709				46709	31448	06^h 35^m 17.60^s	+09Â° 59â² 18.1â³	5.93	â2.50	1583	K4III
HD 52312				52312	33729	07^h 00^m 23.76^s	â08Â° 24â² 24.6â³	5.95	â1.69	1098	B9III
HD 56207				56207	35127	07^h 15^m 43.22^s	â10Â° 35â² 01.0â³	5.95	0.50	401	K0
HD 51814				51814	33603	06^h 58^m 57.03^s	+03Â° 36â² 08.5â³	5.96	â1.31	926	G8III
HD 52913				52913	34002	07^h 03^m 17.93^s	+09Â° 08â² 18.1â³	5.96	1.46	259	A3Vs
HD 58526				58526	36055	07^h 25^m 51.20^s	â05Â° 46â² 29.8â³	5.98	â2.84	1895	G3Ib
T Mon			T	44990	30541	06^h 25^m 13.00^s	+07Â° 05â² 08.6â³	5.98		7762	K1Iabv SB	classical Cepheid, V_max = 5.58^m, V_min = 6.62^m, P = 27.02 d
HD 43319				43319	29711	06^h 15^m 29.66^s	â04Â° 54â² 52.7â³	5.99	1.87	217	A5IVs
HD 61749				61749	37394	07^h 40^m 35.51^s	â08Â° 11â² 07.3â³	6.01	1.12	310	A3IV
HD 55879				55879	34999	07^h 14^m 28.26^s	â10Â° 18â² 58.5â³	6.02	â3.34	2433	B0III
HD 50890				50890	33243	06^h 54^m 58.92^s	â02Â° 48â² 12.9â³	6.03	â1.90	1259	G6III:
Plaskett's star			V640	47129	31646	06^h 37^m 24.04^s	+06Â° 08â² 07.4â³	6.05	â5.49	6618	O8I + O7.5III	one of the most massive spectroscopic binaries known; unique variable, V_max = 6.04^m, V_min = 6.08^m
HD 46178				46178	31168	06^h 32^m 23.27^s	+11Â° 40â² 25.0â³	6.08	â0.96	834	K0III
HD 43362				43362	29705	06^h 15^m 26.16^s	â09Â° 02â² 08.7â³	6.09	â0.76	763	B9III
HD 53929				53929	34338	07^h 07^m 06.48^s	+04Â° 54â² 38.2â³	6.10	â0.59	709	B9.5III
V721 Mon			V721	44816	30407	06^h 23^m 35.92^s	â09Â° 52â² 29.1â³	6.11	â2.88	2050	K5	slow irregular variable
HD 47420				47420	31733	06^h 38^m 20.46^s	â02Â° 32â² 38.1â³	6.14	â0.63	738	K2
1 Mon		1	V474	40535	28321	05^h 59^m 01.07^s	â09Â° 22â² 56.1â³	6.15	1.22	316	F2IV	Î´ Sct variable
HD 42536			V653	42536	29323	06^h 11^m 01.22^s	â06Â° 45â² 15.1â³	6.15	0.01	552	A0sp...	Î±² CVn variable
HD 42278				42278	29210	06^h 09^m 36.21^s	â05Â° 42â² 41.2â³	6.16	2.23	199	F3IVw
HD 45321				45321	30660	06^h 26^m 34.45^s	â04Â° 35â² 50.6â³	6.16	â1.69	1212	B2.5V
HD 45512				45512	30804	06^h 28^m 18.80^s	+10Â° 18â² 14.4â³	6.16	1.74	249	K2III-IV
HR 2517			V715	49567	32682	06^h 49^m 03.66^s	+01Â° 00â² 07.5â³	6.16	â2.75	1976	B3II-III	53 Per variable
HD 63894				63894	38307	07^h 50^m 55.24^s	â11Â° 07â² 42.7â³	6.16	0.66	411	K0
HD 45724				45724	30906	06^h 29^m 14.81^s	+02Â° 38â² 46.6â³	6.17	â0.91	851	M1	suspected variable
HD 45995				45995	31066	06^h 31^m 09.56^s	+11Â° 15â² 05.0â³	6.17	â4.98	5525	B2V:nne	suspected variable
HD 47220				47220	31672	06^h 37^m 40.35^s	+02Â° 42â² 15.4â³	6.17	0.35	475	K1III
V638 Mon			V638	42657	29401	06^h 11^m 43.72^s	â04Â° 39â² 55.6â³	6.18	â0.11	591	B9MNp...	Î±² CVn variable, V_max = 6.16^m, V_min = 6.18^m, P = 0.72 d
HD 48348				48348	32177	06^h 43^m 06.61^s	+03Â° 02â² 01.8â³	6.18	â0.84	827	K0
HD 47886				47886	32012	06^h 41^m 17.22^s	+11Â° 00â² 11.4â³	6.19	â3.27	2547	M1III	semiregular variable
HD 50820				50820	33210	06^h 54^m 42.04^s	â01Â° 45â² 23.3â³	6.20	â4.54	4592	B3IVe+...	suspected variable, V_max = 6.16^m, V_min = 6.28^m
HD 52611				52611	33873	07^h 01^m 52.91^s	â01Â° 20â² 44.8â³	6.20	0.63	424	K0
V731 Mon			V731	47240	31697	06^h 37^m 52.70^s	+04Â° 57â² 24.0â³	6.20		4803	B1Ib	Î± Cyg variable
HD 44037				44037	30028	06^h 19^m 07.94^s	â08Â° 35â² 09.7â³	6.22	0.78	399	B9V
V689 Mon			V689	47432	31766	06^h 38^m 38.19^s	+01Â° 36â² 48.7â³	6.23	â3.86	3396	O9.5II	Î± Cyg variable, V_max = 6.19^m, V_min = 6.26^m, P = 3.55 d
HD 54662				54662	34536	07^h 09^m 20.25^s	â10Â° 20â² 47.7â³	6.23	â5.03	5821	O7III
HD 57708				57708	35737	07^h 22^m 18.59^s	â02Â° 58â² 45.0â³	6.23	â0.06	591	F5
HD 44783				44783	30448	06^h 24^m 02.29^s	+08Â° 53â² 06.1â³	6.24	â0.82	842	B8Vn
HD 59669				59669	36526	07^h 30^m 51.14^s	â05Â° 13â² 35.3â³	6.24	â5.80	8359	K0
HD 51693				51693	33584	06^h 58^m 38.93^s	+07Â° 37â² 20.5â³	6.25	1.93	238	A3V
HD 67159				67159	39675	08^h 06^m 27.42^s	â09Â° 14â² 40.1â³	6.25	â0.68	793	B9V
HD 60853				60853	37000	07^h 36^m 16.67^s	â08Â° 18â² 40.7â³	6.27	â0.13	620	K2	slow irregular variable, V_max = 6.26^m, V_min = 6.29^m
HD 50931				50931	33297	06^h 55^m 34.63^s	+08Â° 19â² 27.4â³	6.28	1.22	335	A0V	variable star, ÎV = 0.005^m, P = 0.49 d
HD 56614				56614	35301	07^h 17^m 31.68^s	â06Â° 40â² 48.1â³	6.29	â2.28	1689	K2	suspected variable
HD 52265				52265	33719	07^h 00^m 18.10^s	â05Â° 22â² 02.5â³	6.3	4.05	91	G0V	CitalÃ¡,^[1] has two planets (b and c)
HD 44333				44333	30217	06^h 21^m 25.78^s	+02Â° 16â² 06.9â³	6.30	1.25	334	A4.5V	Algol variable, V_max = 6.25^m, V_min = 6.33^m
HD 50282				50282	32990	06^h 52^m 22.87^s	â05Â° 18â² 58.5â³	6.30	0.48	477	K0
HD 50371				50371	33082	06^h 53^m 22.40^s	+10Â° 59â² 49.0â³	6.30	0.77	416	K0III
HD 49976			V592	49976	32838	06^h 50^m 42.31^s	â08Â° 02â² 27.6â³	6.31	1.29	330	A2p SrCrEu	Î±² CVn variable, V_max = 6.16^m, V_min = 6.32^m, P = 2.98 d
HD 51424				51424	33420	06^h 57^m 00.10^s	â08Â° 10â² 45.4â³	6.31	â0.93	913	A2V+...
HD 67725				67725	39898	08^h 08^m 56.85^s	â11Â° 20â² 22.7â³	6.31	â0.44	729	A0Vn
HD 45168				45168	30595	06^h 25^m 47.14^s	â03Â° 53â² 20.5â³	6.33	â1.18	1035	G9III
HD 51892				51892	33644	06^h 59^m 20.18^s	+07Â° 19â² 01.2â³	6.34	â1.60	1264	B7III
HD 66242				66242	39326	08^h 02^m 25.97^s	â06Â° 20â² 13.6â³	6.34	1.15	355	G0III
HD 45380				45380	30675	06^h 26^m 44.85^s	â07Â° 30â² 42.9â³	6.35	0.86	409	A0Vn	variable star, ÎV = 0.010^m, P = 21.97 d
HD 48099				48099	32067	06^h 41^m 59.23^s	+06Â° 20â² 43.5â³	6.36		2750	O5.5V((f)) + O9V
HD 50062				50062	32931	06^h 51^m 39.37^s	+03Â° 02â² 31.4â³	6.37	1.57	298	A2Vs
HD 45090				45090	30602	06^h 25^m 52.33^s	+11Â° 07â² 33.3â³	6.39	0.67	454	A0
HD 47156				47156	31662	06^h 37^m 36.92^s	+10Â° 51â² 12.1â³	6.39	â0.77	883	K0
HD 50700				50700	33154	06^h 54^m 08.60^s	â05Â° 51â² 07.9â³	6.39	0.21	562	A6Vn
HD 45239				45239	30608	06^h 25^m 58.83^s	â07Â° 53â² 41.9â³	6.40	0.24	556	A4V
HD 66950				66950	39625	08^h 05^m 49.64^s	â00Â° 34â² 24.0â³	6.40	â0.30	712	K0	suspected variable
HD 44700				44700	30382	06^h 23^m 18.49^s	+03Â° 45â² 52.2â³	6.41	â1.23	1098	B3V	variable star, ÎV = 0.010^m, P = 31.10 d
V695 Mon			V695	65875	39172	08^h 00^m 44.14^s	â02Â° 52â² 54.9â³	6.42	â3.48	3105	B2.5Ve	Î³ Cas variable, V_max = 6.42^m, V_min = 6.53^m
HD 45215				45215	30627	06^h 26^m 09.60^s	â03Â° 30â² 57.1â³	6.42	0.34	536	G5
24 Mon		24		56003	35080	07^h 15^m 19.41^s	â00Â° 09â² 40.7â³	6.42	0.36	530	G5III
HD 57682				57682	35707	07^h 22^m 02.05^s	â08Â° 58â² 45.9â³	6.42	â4.03	4009	O9V	suspected variable, V_max = 6.34^m, V_min = 6.45^m
14 Mon		14		46642	31385	06^h 34^m 46.33^s	+07Â° 34â² 21.0â³	6.44	1.21	362	A0Vs	suspected variable
HD 53240				53240	34066	07^h 03^m 57.46^s	â10Â° 07â² 25.6â³	6.44	â1.52	1273	B9IIIn
HD 65938				65938	39198	08^h 01^m 03.45^s	â06Â° 25â² 08.7â³	6.45	2.33	217	G5
HD 42132				42132	29140	06^h 08^m 47.72^s	â06Â° 49â² 17.0â³	6.46	1.23	363	G5
HD 45563				45563	30798	06^h 28^m 16.77^s	+01Â° 54â² 45.8â³	6.48	0.60	489	B9V
HD 52382				52382	33754	07^h 00^m 39.34^s	â09Â° 12â² 10.7â³	6.49	â3.28	2937	B1Ib	suspected variable, V_max = 6.47^m, V_min = 6.5^m
9 Mon		9		45418	30700	06^h 27^m 00.88^s	â04Â° 21â² 20.3â³	6.50	â1.10	1079	B4V
V569 Mon			V569	53755	34234	07^h 05^m 49.64^s	â10Â° 39â² 36.3â³	6.50	â3.68	3543	B0.5IVn	Î² Cep variable, V_max = 6.42^m, V_min = 6.53^m, P = 0.27 d
IM Mon			IM	44701	30351	06^h 23^m 01.47^s	â03Â° 16â² 37.1â³	6.54		991	B5V	Î² Lyr variable
HD 50281A				50281	32984	06^h 52^m 18.05^s	â05Â° 10â² 25.4â³	6.57		28.395	K3.5V	component of the HD 50281 system
V926 Mon			V926	52690	33891	07^h 02^m 06.73^s	â03Â° 45â² 17.4â³	6.62		1920	M1Ib	semiregular variable, V_max = 6.50^m, V_min = 6.70^m, P = 39 d
HD 50138			V743	50138	32923	06^h 51^m 33.40^s	â06Â° 57â² 59.5â³	6.67		1280	B9e	FS CMa variable, V_max = 6.53^m, V_min = 6.87^m
Îµ Mon B	Îµ			44770	30422	06^h 23^m 46.50^s	+04Â° 35â² 45.1â³	6.72	4.79	79	F5V	component of the Îµ Mon system
HD 46150				46150	31130	06^h 31^m 55.52^s	+04Â° 56â² 34.3â³	6.75		5200	O5V((f))	in NGC 2244; variable star, ÎV = 0.008^m
6 Mon		6		43760	29885	06^h 17^m 35.13^s	â10Â° 43â² 30.0â³	6.76	â0.87	1094	F0e...
AX Mon			AX	45910	31019	06^h 30^m 32.94^s	+05Â° 52â² 01.2â³	6.85		12000	B2IIIe	unique variable, V_max = 6.59^m, V_min = 6.94^m, P = 232.5 d
HD 46966				46966	31567	06^h 36^m 25.89^s	+06Â° 04â² 59.5â³	6.87			O8V	variable star, ÎV = 0.006^m
V Mon			V	44639	30326	06^h 22^m 43.50^s	â02Â° 11â² 42.0â³	6.87		2194	M6e	Mira variable, V_max = 6^m, V_min = 13.9^m, P = 340.5 d
V644 Mon			V644	51480	33436	06^h 57^m 09.38^s	â10Â° 49â² 28.1â³	6.93		4900	Ape	Î³ Cas variable, V_max = 6.88^m, V_min = 6.98^m
HD 53367			V750	53367	34116	07^h 04^m 25.53^s	â10Â° 27â² 15.7â³	6.96		932	B0IV:e	Î³ Cas variable, V_max = 6.92^m, V_min = 7.22^m
Gliese 282 A			V869	61606	37349	07^h 39^m 59.33^s	â03Â° 35â² 51.0â³	7.18		46.33	K2V	component of the Gliese 282 system; BY Dra variable, ÎV = 0.02^m
V505 Mon			V505	48914	32397	06^h 45^m 49.98^s	+02Â° 29â² 57.4â³	7.22		2170	B5Ib	Î² Lyr variable, V_max = 7.15^m, V_min = 7.65^m, P = 53.78 d
V614 Mon			V614	52432	33794	07^h 01^m 01.95^s	â03Â° 15â² 09.1â³	7.27		1550	C...	semiregular variable, V_max = 7.01^m, V_min = 7.36^m, P = 60 d
HD 46223				46223	31149	06^h 32^m 09.31^s	+04Â° 49â² 24.7â³	7.28		5200	O5e	in NGC 2244; variable star, ÎV = 0.008^m
HD 46149				46149	31128	06^h 31^m 52.53^s	+05Â° 01â² 59.2â³	7.61		5200	O8.5V+B	in NGC 2244; spectroscopic binary; rotating and pulsating variable
HD 44219				44219	30114	06^h 20^m 14.32^s	â10Â° 43â² 30.0â³	7.70	4.19	164	G5	has a planet (b)
HD 46375				46375	31246	06^h 33^m 12.62^s	+05Â° 27â² 46.5â³	7.84	5.22	109	K1V	has a planet (b)
HD 59435			V827	59435	36419	07^h 29^m 35.45^s	â09Â° 15â² 33.3â³	7.97		1210	A5p	Î±² CVn variable, V_max = 7.97^m, V_min = 7.99^m, P = 3.59 d
HD 45583			V682	45583	30789	06^h 28^m 10.76^s	â04Â° 53â² 56.5â³	7.97		962	B9	Î±² CVn variable
HD 46380			V728	46380	31199	06^h 32^m 43.23^s	â07Â° 30â² 32.3â³	8.00		1480	B2Vne	Be star
HD 45652				45652	30905	06^h 29^m 13.19^s	+10Â° 56â² 02.0â³	8.13	5.34	118	G8-K0	LusitÃ¢nia,^[2] has a planet (b)
HD 46202				46202		06^h 32^m 10.47^s	+04Â° 57â² 59.8â³	8.18		5200	O9V	in NGC 2244; Î² Cep variable, ÎV = 0.01^m, P = 0.21 d
HD 66428				66428	39417	08^h 03^m 28.67^s	â01Â° 09â² 45.8â³	8.25	4.55	180	G5	has a planet (b)
V753 Mon			V753	54975	34684	07^h 10^m 57.85^s	â03Â° 52â² 43.2â³	8.27		605	A8V	Algol variable, V_max = 8.30^m, V_min = 8.81^m, P = 0.68 d
V723 Mon			V723	45762	30891	06^h 29^m 04.66^s	â05Â° 34â² 20.2â³	8.28		1700	G0II	Long period variable, potential black hole binary
SV Mon			SV	44320	30219	06^h 21^m 26.30^s	+06Â° 28â² 12.6â³	8.28			G7II...	classical Cepheid, V_max = 7.61^m, V_min = 8.88^m, P = 15.23 d
HD 50064				50064		06^h 51^m 34.11^s	+00Â° 17â² 50.4â³	8.30		9500	B6:Ia	one of the most luminous stars known; Î± Cyg variable, V_max = 8.02^m, V_min = 8.41^m, P = 60 d
HD 47755			V684	47755		06^h 40^m 38.30^s	+09Â° 47â² 15.8â³	8.41			B4	Algol variable, V_max = 8.32^m, V_min = 8.41^m, P = 1.85 d
UX Mon			UX	65607	39042	07^h 59^m 16.38^s	â07Â° 30â² 17.9â³	8.42		5500	A3	Algol and Î´ Sct variable, V_max = 8.22^m, V_min = 9.16^m, P = 5.90 d
AU Mon			AU	50846	33237	06^h 54^m 54.71^s	â01Â° 22â² 32.8â³	8.43			B5IV + F8-G0III-II	double periodic or Algol variable, V_max = 8.20^m, V_min = 9.16^m, P = 11.11 d
HD 47732			V641	47732	31939	06^h 40^m 28.59^s	+09Â° 49â² 04.3â³	8.46		2190	B3Vnn...	rotating ellipsoidal variable, ÎV = 0.07^m, P = 1.32 d
V578 Mon			V578	259135		06^h 32^m 00.61^s	+04Â° 52â² 40.9â³	8.55			B1:V:n	Algol variable, V_max = 8.54^m, V_min = 8.57^m, P = 2.41 d
HD 259431			V700	259431	31235	06^h 33^m 05.19^s	+10Â° 19â² 20.0â³	8.72		564	B6ep	Orion variable, V_max = 8.62^m, V_min = 8.91^m
AR Mon			AR	57364	35600	07^h 20^m 48.45^s	â05Â° 15â² 35.8â³	8.79		962	K0II	RS CVn variable, V_max = 8.62^m, V_min = 9.47^m, P = 21.21 d
Gliese 282 B				61606B		07^h 40^m 02.88^s	â03Â° 36â² 13.4â³	8.93		46.33	K7V +	component of the Gliese 282 system
HD 44179			V777	44179	30089	06^h 19^m 58.22^s	â10Â° 38â² 14.7â³	8.94		1245	B8V	central star of Red Rectangle Nebula; re-radiating binary system, V_max = 8.78^m, V_min = 8.94^m, P = 320 d
HD 49330			V739	49330	32586	06^h 47^m 57.27^s	+00Â° 46â² 34.0â³	8.95		1460	B0.5IVe	Î³ Cas variable, V_max = 8.72^m, V_min = 9.02^m
HD 50169				50169	32965	06^h 51^m 59.23^s	â01Â° 38â² 40.4â³	8.99	1.69	1489	A4p	Brewer's Star
FU Mon			FU	44544	30301	06^h 22^m 23.85^s	+03Â° 25â² 27.9â³	9.06		2490	S6.5/7.5	semiregular variable
TU Mon			TU		38523	07^h 53^m 19.75^s	â03Â° 02â² 31.1â³	9.24		1960	B5V + F3	Algol variable
RW Mon			RW	259986	31383	06^h 34^m 45.89^s	+08Â° 49â² 32.18â³	9.32		738	B8V + G5IV	Algol variable, V_max = 9.26^m, V_min = 11.51^m, P = 1.91 d
VV Mon			VV		34003	07^h 03^m 18.29^s	â05Â° 44â² 15.5â³	9.40		434	G0	RS CVn variable, V_max = 9.4^m, V_min = 9.95^m, P = 6.05 d
BX Mon			BX			07^h 25^m 22.78^s	â03Â° 35â² 15.8â³	9.50			M5IIIpe	Z And variable, V_max = 9.5^m, V_min = 12.5^m, P = 1259 d
PZ Mon			PZ	289114	32621	06^h 48^m 21.07^s	+01Â° 13â² 08.3â³	9.60		2080	K2Ve	irregular variable
V694 Mon			V694			07^h 25^m 51.29^s	â07Â° 44â² 08.1â³	9.70		1550	C...	Z And variable, V_max = 9.2^m, V_min = 11.4^m, P = 1931 d
AO Mon			AO	53883	34299	07^h 06^m 36.30^s	â04Â° 37â² 24.5â³	9.72			B3 + B5	Algol and Î´ Sct variable, V_max = 9.6^m, V_min = 10.23^m, P = 1.88 d
V588 Mon			V588	261331		06^h 39^m 05.90^s	+09Â° 41â² 03.4â³	9.75			A7III/IV	Î´ Sct variable, V_max = 9.66^m, V_min = 9.72^m, P = 0.11 d
V372 Mon			V372			06^h 41^m 26.13^s	â04Â° 35â² 45.8â³	9.81			SC7/7.5	semiregular variable
CV Mon			CV		31624	06^h 37^m 04.84^s	+03Â° 03â² 50.2â³	9.90				in C0634+031; classical Cepheid, V_max = 9.9^m, V_min = 10.7^m, P = 5.38 d
G 112-29					36985	07^h 36^m 07.08^s	â03Â° 06â² 38.8â³	9.99		46.21	M:	component of the Gliese 282 system; rotating variable, V_max = 0.19^m, V_min = 12.16^m
HD 50281B				50281B		06^h 52^m 18.05^s	â05Â° 11â² 24.2â³	10.05			M2	component of the HD 50281 system
V589 Mon			V589	261446		06^h 39^m 28.46^s	+09Â° 42â² 04.1â³	10.27			F2III	Î´ Sct variable, ÎV = 0.05^m, P = 0.12 d
BE Mon			BE		31905	06^h 40^m 05.58^s	+07Â° 36â² 21.0â³	10.5			G5	classical Cepheid, V_max = 10.19^m, V_min = 10.88^m, P = 2.71 d
RU Mon			RU		33163	06^h 54^m 12.31^s	â07Â° 35â² 45.0â³	10.51			B9pv + B7V + B7.2V	Algol variable, V_max = 10.33^m, V_min = 11.18^m, P = 3.58 d
CL Mon			CL			06^h 55^m 36.70^s	+06Â° 22â² 43.3â³	11.00			C...	Mira variable, V_max = 8.1^m, V_min = 13.0^m, P = 493 d
Ross 614			V577		30920	06^h 29^m 23.40^s	â02Â° 48â² 50.3â³	11.08	13.01	13.4	M4.5V + M8V	binary star; one component is a flare star
DD Mon			DD	292319		06^h 45^m 57.83^s	â00Â° 07â² 31.9â³				G0	Algol variable
A0620-00			V616			06^h 22^m 44.50^s	â00Â° 20â² 44.7â³	11.2			K3V-K7V	X-ray nova and rotating ellipsoidal variable, V_max = 11.0^m, V_min = 18.3^m, P = 0.32 d
CS Mon			CS			06^h 32^m 10.94^s	+06Â° 39â² 11.0â³	11.25				classical Cepheid, V_max = 10.71^m, V_min = 11.3^m, P = 6.73 d
COROT-7						06^h 43^m 49.47^s	â01Â° 03â² 46.9â³	11.73	5.85	489	K0V	has two planets (b & c) and one unconfirmed planet (d)
R Mon			R			06^h 39^m 09.95^s	+08Â° 44â² 10.8â³	11.85			B0	in NGC 2261; Orion variable
BN Mon			BN			06^h 21^m 58.00^s	+07Â° 20â² 57.7â³	12.70			Nv...	semiregular variable
V396 Mon			V396			06^h 38^m 36.48^s	+03Â° 36â² 17.1â³					W UMa variable
V590 Mon			V590			06^h 40^m 44.64^s	+09Â° 48â² 02.1â³	12.88			B7	Orion variable
COROT-4						06^h 48^m 46.70^s	â00Â° 40â² 22.0â³	13.45			F0V	has a transiting planet (b)
COROT-1						06^h 48^m 19.17^s	â03Â° 06â² 07.8â³	13.6	5.2	1560	G0V	first transiting planet by COROT mission (b)
VY Mon			VY			06^h 31^m 06.92^s	+10Â° 26â² 05.0â³	13.70			B8	UX Ori star
COROT-5						06^h 45^m 06.54^s	+00Â° 48â² 54.9â³	14	6	1300	F9V	has a transiting planet (b)
COROT-20						06^h 30^m 53^s	+00Â° 13â² 37â³	14.66		4012	G2V	has a transiting planet (b)
COROT-19						06^h 28^m 08^s	â00Â° 01â² 01â³	14.78		2609	F9V	has a transiting planet (b)
COROT-18						06^h 32^m 41^s	â00Â° 01â² 54â³	14.99		2838	G9	has a transiting planet (b)
COROT-13						06^h 50^m 53.07^s	â05Â° 05â² 11.1â³	15.04	4.45	4270	G0V	has a transiting planet (b)
BT Mon			BT			06^h 43^m 47.24^s	â02Â° 01â² 13.9â³	15.4			G5V	nova and Algol variable, V_max = 4.5^m, V_min = 16.4^m, P = 0.33 d
COROT-12						06^h 43^m 03.76^s	â01Â° 17â² 47.1â³	15.52	5.21	3760	G2V	has a transiting planet (b)
V838 Mon			V838			07^h 04^m 04.85^s	â03Â° 50â² 51.1â³	15.74		20000	M6I/III + B3V	luminous red nova, V_max = 6.7^m, V_min = 16.05^m
COROT-14						06^h 53^m 41.80^s	â05Â° 32â² 09.7â³	16.03	5.40	4360	F9V	has a transiting planet (b)
CW Mon			CW			06^h 36^m 54.58^s	+00Â° 02â² 17.3â³	17.2		5500	A3	SS Cyg variable, V_max = 11.9^m, V_min = 17.2^m, P = 0.18 d
Scholz's Star						07^h 20^m 03.25^s	â08Â° 46â² 49.9â³	18.3	19.4	19.65	M9.5+T5C	Binary star
AFGL 961						06^h 34^m 37.63^s	+04Â° 12â² 42.8â³				K3V-K7V	young stellar object
Monoceros R2 IRS 3						06^h 47^m 47.8^s	â06Â° 22â² 55â³					young stellar object
NGC 2264 IRS 1						06^h 41^m 10.06^s	+09Â° 29â² 35.8â³				B2	in NGC 2264; young stellar object
UGPS J072227.51-054031.2						07^h 22^m 27.87^s	â05Â° 40â² 31.1â³			13	T9	brown dwarf

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[1]

[2]

List of stars in Monoceros

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References

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