NGC 4744
Centaurus | |
---|---|
Right ascension | 12h 52m 19.6s[1] |
Declination | −41° 03′ 36″[1] |
Redshift | 0.011201[1] |
Heliocentric radial velocity | 3358 km/s[1] |
Distance | 162 Mly (49.7 Mpc)[1] |
Group or cluster | Centaurus Cluster |
Apparent magnitude (V) | 13.77[1] |
Characteristics | |
Type | SB0/a(s)[1] |
Size | ~145,400 ly (44.59 kpc) (estimated)[1] |
Apparent size (V) | 2.1 x 1.0[1] |
Other designations | |
ESO 323-22, CCC 227, IRAS 12495-4047, MCG -7-27-6, PGC 43661[1] |
NGC 4744 is a
barred lenticular galaxy located about 160 million light-years away[2] in the constellation Centaurus.[3] NGC 4744 was discovered by astronomer John Herschel on June 8, 1834.[4] It is a member of the Centaurus Cluster.[5][6]
See also
References
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4744. Archived from the original on 2000-10-19. Retrieved 2018-04-16.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Archived from the original on 2022-12-18. Retrieved 2018-04-16.
- ^ "Revised NGC Data for NGC 4744". spider.seds.org. Archived from the original on 2016-05-27. Retrieved 2018-04-16.
- ^ "New General Catalog Objects: NGC 4700 - 4749". cseligman.com. Archived from the original on 2018-04-11. Retrieved 2018-04-11.
- ISSN 0365-0138.
- ISBN 978-1-139-85154-1. Archivedfrom the original on 2024-05-03. Retrieved 2018-04-16.
External links
- NGC 4744 on