List of stars in Canis Major

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

List

Zdroj:https://en.wikipedia.org?pojem=List_of_stars_in_Canis_Major
Text je dostupný za podmienok Creative Commons Attribution/Share-Alike License 3.0 Unported; prípadne za ďalších podmienok. Podrobnejšie informácie nájdete na stránke Podmienky použitia.

Navigácia: Veda >

Analytika
Antropológia
Aplikované vedy
Bibliometria
Dejiny vedy
Encyklopédie
Filozofia vedy
Forenzné vedy
Humanitné vedy
Knižničná veda
Kryogenika
Kryptológia
Kulturológia
Literárna veda
Medzidisciplinárne oblasti
Metódy kvantitatívnej analýzy
Metavedy
Metodika

Metodológia vedy
Náboženstvo a veda
Náučná literatúra
Podvody vo vede
Popularizácia vedy
Potravinárstvo
Prírodné vedy
Pseudoveda
Scientometria
Spoločenské vedy
Teórie
Teatrológia
Technické vedy
Technika
Terminológia
Umenie
Výskum

Veda
Veda a technika podľa štátu
Veda a technika podľa kontinentu
Veda a technika podľa roka
Veda v kozme
Vedci
Vedecká literatúra
Vedecké databázy
Vedecké experimenty
Vedecké konferencie
Vedecké metódy
Vedecké ocenenia
Vedecké organizácie
Vedecké parky
Vedeckí spisovatelia
Vzdelávanie
Záhady

Príbuzné výrazy:

Text je dostupný za podmienok Creative Commons Attribution/Share-Alike License 3.0 Unported; prípadne za ďalších podmienok.
Podrobnejšie informácie nájdete na stránke Podmienky použitia.

Name	B	F	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
Sirius A, B	α	9		48915	32349	06^h 45^m 09.25^s	−16° 42′ 47.3″	−1.46	1.42	8.6	A0m...	Alhabor, Aschere, Canicula, the Dog Star; brightest star, 5th nearest star system; binary
ε CMa	ε	21		52089	33579	06^h 58^m 37.55^s	−28° 58′ 19.5″	1.50	−4.10	431	B2II	Adhara, Aoul al Adzari, Prima Virginum^[1] part of Al ʽAdhārā or Al Adzari^[2]^[3]
δ CMa	δ	25		54605	34444	07^h 08^m 23.49^s	−26° 23′ 35.5″	1.83	−6.87	1791	F8Ia	Wezen, Thalath al Adzari, Tertia Virginum,^[1] part of Al ʽAdhārā or Al Adzari;^[2]^[3] variable star, ΔV = 0.004^m, P = 24.08478 d
β CMa	β	2		44743	30324	06^h 22^m 41.99^s	−17° 57′ 21.3″	1.98	−3.95	499	B1II/III	Mirzam (Murzim); β Cep variable, V_max = 1.93^m, V_min = 2^m, P = 0.25003 d
η CMa	η	31		58350	35904	07^h 24^m 05.71^s	−29° 18′ 11.2″	2.45	−7.51	3196	B5Ia	Aludra, part of Al ʽAdhārā or Al Adzari;^[2]^[3] α Cyg variable
ζ CMa	ζ	1		44402	30122	06^h 20^m 18.79^s	−30° 03′ 48.2″	3.02	−2.05	336	B2.5V	Furud; spectroscopic binary; suspected variable
ο² CMa	ο²	24		53138	33977	07^h 03^m 01.47^s	−23° 49′ 59.9″	3.02	−6.46	2567	B3Ia	Thanih al Adzari, Secunda Virginum,^[1] part of Al ʽAdhārā or Al Adzari;^[2]^[3] α Cyg variable
σ CMa	σ	22		52877	33856	07^h 01^m 43.15^s	−27° 56′ 05.4″	3.49	−4.37	1216	K4III	Unurgunite, irregular variable, V_max = 3.43^m, V_min = 3.51^m
κ CMa	κ	13		50013	32759	06^h 49^m 50.47^s	−32° 30′ 30.6″	3.50	−3.42	789	B1.5IVne	γ Cas variable, V_max = 3.40^m, V_min = 3.97^m
ο¹ CMa	ο¹	16		50877	33152	06^h 54^m 07.95^s	−24° 11′ 03.2″	3.89	−5.02	1976	K3Iab	irregular variable, V_max = 3.78^m, V_min = 3.99^m
ν² CMa	ν²	7		47205	31592	06^h 36^m 41.00^s	−19° 15′ 20.6″	3.95	2.46	65	K1III+...	Yějī (野雞),^[4] has a planet (b); suspected variable, V_max = 3.87^m, V_min = 3.96^m
ω CMa	ω	28		56139	35037	07^h 14^m 48.66^s	−26° 46′ 21.7″	4.01	−3.25	924	B2IV/Ve	γ Cas variable, V_max = 3.54^m, V_min = 4.18^m
θ CMa	θ	14		50778	33160	06^h 54^m 11.48^s	−12° 02′ 18.9″	4.08	−0.36	252	K4III
γ CMa	γ	23		53244	34045	07^h 03^m 45.49^s	−15° 37′ 59.7″	4.12	−1.34	402	B8II	Muliphein; suspected variable
ξ¹ CMa	ξ¹	4		46328	31125	06^h 31^m 51.37^s	−23° 25′ 06.4″	4.34	−4.65	2050	B1III	β Cep variable, V_max = 4.33^m, V_min = 4.36^m, P = 0.2095755 d
ι CMa	ι	20		51309	33347	06^h 56^m 08.23^s	−17° 03′ 15.3″	4.36	−5.51	3075	B3Ib/II	β Cep variable, V_max = 4.36^m, V_min = 4.4^m, P = 0.08 d
τ CMa	τ	30		57061	35415	07^h 18^m 42.49^s	−24° 57′ 15.8″	4.37	−5.59	3196	O9Ib	member of the NGC 2362 star cluster; β Lyr variable
ν³ CMa	ν³	8		47442	31700	06^h 37^m 53.43^s	−18° 14′ 14.8″	4.42	−1.35	464	K0II/III
27 CMa		27	EW	56014	34981	07^h 14^m 15.22^s	−26° 21′ 09.1″	4.42	−4.00	1575	B3IIIe	binary, component A spectroscopic binary, component B γ Cas variable, V_max = 4.42^m, V_min = 4.82^m
λ CMa	λ			45813	30788	06^h 28^m 10.22^s	−32° 34′ 48.5″	4.47	−1.01	406	B4V
ξ² CMa	ξ²	5		46933	31416	06^h 35^m 03.38^s	−22° 57′ 53.4″	4.54	−0.97	412	A0III
π CMa	π	19		51199	33302	06^h 55^m 37.40^s	−20° 08′ 11.7″	4.66	2.33	95	F2IV/V	variable star, ΔV = 0.002^m, P = 0.09013 d
HD 56618				56618	35205	07^h 16^m 35.00^s	−27° 52′ 52.6″	4.66	−1.05	453	M2III	suspected variable
HD 47667				47667	31827	06^h 39^m 16.72^s	−14° 08′ 44.7″	4.82	−3.60	1575	K2III
15 CMa		15	EY	50707	33092	06^h 53^m 32.91^s	−20° 13′ 27.3″	4.82	−3.65	1614	B1IV	β Cep variable, V_max = 4.79^m, V_min = 4.84^m, P = 0.184557 d
HD 56577^[5]				56577	35210	07^h 16^m 36.84^s	−23° 18′ 56.2″	4.83	−6.59	6269	K4III	Double star; suspected variable, V_max = 4.78^m, V_min = 4.86^m
UW CMa		29	UW	57060	35412	07^h 18^m 40.38^s	−24° 33′ 31.3″	4.88	−4.93	2991	O7Ia:fp	β Lyr variable, V_max = 4.84^m, V_min = 5.33^m, P = 4.393407 d
HD 57821				57821	35727	07^h 22^m 13.53^s	−19° 00′ 59.7″	4.94	−1.06	517	B5II/III
HD 43445				43445	29735	06^h 15^m 44.88^s	−13° 43′ 06.2″	5.00	−0.30	375	B9V
μ CMa	μ	18		51250	33345	06^h 56^m 06.65^s	−14° 02′ 36.4″	5.00	−2.22	908	B9.5V	Isis
HD 43827				43827	29895	06^h 17^m 41.73^s	−16° 48′ 57.3″	5.15	−1.05	567	K1III
HD 46184				46184	31084	06^h 31^m 23.02^s	−12° 23′ 30.9″	5.16	0.05	343	K1III
HD 58343			FW	58343	35951	07^h 24^m 40.19^s	−16° 12′ 05.1″	5.18	−2.13	945	B2Vne	γ Cas variable, V_max = 5.^m, V_min = 5.5^m
HD 44951				44951	30457	06^h 24^m 10.35^s	−11° 31′ 48.0″	5.21	−0.34	420	K3III
10 CMa		10	FT	48917	32292	06^h 44^m 28.47^s	−31° 04′ 13.9″	5.23	−4.29	2608	B2V	γ Cas variable, V_max = 5.13^m, V_min = 5.44^m
HD 47536				47536	31688	06^h 37^m 47.54^s	−32° 20′ 23.6″	5.25	−0.17	396	K1III	has two planets (b & c)
11 CMa		11		49229	32492	06^h 46^m 51.09^s	−14° 25′ 33.6″	5.28	−1.19	642	B8/B9III
HD 51283				51283	33316	06^h 55^m 46.93^s	−22° 56′ 29.2″	5.28	−3.82	2159	B2/B3III	suspected variable
HD 57146				57146	35427	07^h 18^m 51.28^s	−26° 35′ 09.1″	5.29	−2.80	1353	G2II	suspected variable
HD 49048				49048	32411	06^h 45^m 59.40^s	−14° 47′ 45.9″	5.30	−0.13	398	A1IV/V
HD 58535				58535	35957	07^h 24^m 43.87^s	−31° 48′ 32.1″	5.35	−0.79	552	K1III	suspected variable, V_max = 5.31^m, V_min = 5.43^m
HD 56342				56342	35083	07^h 15^m 21.08^s	−30° 41′ 11.3″	5.36	−1.12	646	B2V	suspected variable, ΔV = 0.006^m
HD 58215				58215	35848	07^h 23^m 28.97^s	−27° 50′ 03.4″	5.37	−0.76	549	K4III	variable star, ΔV = 0.008^m, P = 20.67397 d
HD 49662				49662	32677	06^h 48^m 57.74^s	−15° 08′ 41.0″	5.39	−0.96	607	B7IV	variable star, ΔV = 0.010^m, P = 1.43019 d
NO CMa			NO	58155	35795	07^h 23^m 00.70^s	−31° 55′ 25.6″	5.40	−2.81	1430	B3V	Be star
FN CMa			FN	53974	34301	07^h 06^m 40.77^s	−11° 17′ 38.5″	5.41	−4.29	2835	B0.5IV	β Cep variable, V_max = 5.38^m, V_min = 5.42^m, P = 0.08866 d
HD 58286				58286	35855	07^h 23^m 31.90^s	−32° 12′ 07.5″	5.41	−2.34	1156	B2/B3II/III
HD 51733				51733	33478	06^h 57^m 33.97^s	−24° 37′ 51.8″	5.45	2.52	126	F3V
HD 55070				55070	34624	07^h 10^m 19.33^s	−27° 29′ 29.5″	5.46	−1.01	643	G8III
HD 56405				56405	35180	07^h 16^m 14.58^s	−15° 35′ 08.4″	5.46	0.82	277	A1V	suspected variable
FR CMa			FR	44458	30214	06^h 21^m 24.72^s	−11° 46′ 23.7″	5.48	−3.07	1672	B1Vpe SB	γ Cas variable, V_max = 5.46^m, V_min = 5.64^m
HD 43955				43955	29941	06^h 18^m 13.73^s	−19° 58′ 01.2″	5.51	−1.91	994	B2/B3V
HD 56160				56160	35044	07^h 14^m 51.19^s	−27° 02′ 16.5″	5.58	0.97	273	K3III	variable star, ΔV = 0.006^m, P = 4.45653 d
HD 52018				52018	33575	06^h 58^m 35.90^s	−25° 24′ 51.0″

[1]

[2]

[3]

[4]

[5]