Messier 49
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Observation data: J2000 epoch | |
---|---|
Constellation: | Virgo |
Right ascension: | 12h 29m 46.7s[1] |
Declination: | +08° 00′ 02″[1] |
Redshift: | 997 ± 7 km/s[1] |
Distance: | 53 ± 2 Mly (16.3 ± 0.8 Mpc)[2] |
Type: | E2/S0[1] |
Apparent dimensions (V): | 10′.2 × 8′.3[1] |
Apparent magnitude (V): | 9.4[1] |
Notable features: | |
Other designations | |
NGC 4472,[1] UGC 7629,[1] PGC 41220,[1] Arp 134[1] | |
See also: Galaxy, List of galaxies |
Messier 49 (also known as M 49 or NGC 4472) is an elliptical / lenticular galaxy about 53 million light-years away in the constellation Virgo. The galaxy was discovered by Charles Messier in 1771[3].
Contents |
[edit] Supernovae
The only supernova observed within this galaxy is SN 1969Q[4]. The supernova was discovered in June 1969[5].
[edit] Companion galaxies
NGC 4467 forms a visual pair with Messier 49[citation needed].
[edit] Virgo Cluster membership
Messier 49 is the brightest member of the Virgo Cluster[6]. The galaxy is located at the center of one of the subclusters within the Virgo Cluster[6].
[edit] External links
[edit] References
- ^ a b c d e f g h i j NASA/IPAC Extragalactic Database. Results for NGC 4472. Retrieved on September 26, 2006.
- ^ J. L. Tonry, A. Dressler, J. P. Blakeslee, E. A. Ajhar, A. B. Fletcher, G. A. Luppino, M. R. Metzger, C. B. Moore (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal 546 (2): 681-693.
- ^ K. G. Jones (1991). Messier's Nebulae and Star Clusters, 2nd edition, Cambridge: Cambridge University Press. ISBN 0-521-37079-5.
- ^ NASA/IPAC Extragalactic Database. Results for supernova search near name "NGC 4472". Retrieved on February 12, 2007.
- ^ R. Barbon, E. Cappellaro, F. Ciatti, M. Turatto, C. T. Kowal (1984). "A revised supernova catalogue". Astronomy & Astrophysics Supplement Series 58: 735-750.
- ^ a b A. Sandage, J. Bedke (1994). Carnegie Atlas of Galaxies. Washington, D.C.: Carnegie Institution of Washington. ISBN 0-87279-667-1.