Revision as of 14:33, 7 September 2017 editCydebot (talk | contribs)6,812,251 editsm Robot - Moving category Canes Venatici (constellation) to Category:Canes Venatici per CFD at Misplaced Pages:Categories for discussion/Log/2017 August 14.← Previous edit | Revision as of 06:33, 9 September 2017 edit undoBibcode Bot (talk | contribs)Bots42,789 editsm Adding 1 arxiv eprint(s), 0 bibcode(s) and 0 doi(s). Did it miss something? Report bugs, errors, and suggestions at User talk:Bibcode BotNext edit → | ||
Line 25: | Line 25: | ||
| journal=Publications of the Astronomical Society of Australia | | journal=Publications of the Astronomical Society of Australia | ||
| volume=25 | issue=4 | pages=167-175 | date=November 2008 | | volume=25 | issue=4 | pages=167-175 | date=November 2008 | ||
| doi=10.1071/AS08013 | bibcode=2008PASA...25..167G }}</ref> | | doi=10.1071/AS08013 | bibcode=2008PASA...25..167G |arxiv = 0807.2549 }}</ref> | ||
==History== | ==History== |
Revision as of 06:33, 9 September 2017
Messier 63 | |
---|---|
M63 from GALEX sky survey | |
Observation data (J2000 epoch) | |
Constellation | Canes Venatici |
Right ascension | 13 15 49.3 |
Declination | +42° 01′ 45″ |
Redshift | 484 km/s |
Distance | 27 Mly |
Apparent magnitude (V) | 9.3 |
Characteristics | |
Type | SA(rs)bc |
Apparent size (V) | 12′.6 × 7′.2 |
Other designations | |
M63, NGC 5055, UGC 8334, PGC 46153 |
Messier 63 (also known as M63, NGC 5055, or the Sunflower Galaxy) is a spiral galaxy in the constellation Canes Venatici consisting of a central disc surrounded by many short spiral arm segments. M63 is part of the M51 Group, a group of galaxies that also includes M51 (the 'Whirlpool Galaxy'). M63 is an active galaxy with a LINER nucleus. The existence of a super massive black hole (SMBH) at the nucleus is uncertain; if it does exist, then the mass is estimated as (8.5±1.9)×10 M☉.
History
M63 was discovered by Pierre Méchain on June 14, 1779. The galaxy was then listed by Charles Messier as object 63 in the Messier Catalogue.
In the mid-19th century, Lord Rosse identified spiral structures within the galaxy, making this one of the first galaxies in which such structure was identified.
In 1971, a supernova with a magnitude of 11.8 appeared in one of the arms of M63.
References
- ^ "NASA/IPAC Extragalactic Database". Results for NGC 5055. Retrieved 2006-10-10.
- NASA (2015). . Retrieved Mar. 2, 2017
- "M 63". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 November 2015.
- Graham, Alister W. (November 2008), "Populating the Galaxy Velocity Dispersion - Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values", Publications of the Astronomical Society of Australia, 25 (4): 167–175, arXiv:0807.2549, Bibcode:2008PASA...25..167G, doi:10.1071/AS08013.
- ^ K. G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge: Cambridge University Press. ISBN 0-521-37079-5.
External links
- The Sunflower Galaxy on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- Sunflower Galaxy @ SEDS Messier pages
- Sunflower Galaxy (M63) at Constellation Guide
Messier objects | ||
---|---|---|
List |
| |
See also | ||