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'''Messier 63''' (also known as '''M63''', '''NGC 5055''', or the '''Sunflower Galaxy''') is a ] in the ] ] consisting of a central disc surrounded by many short spiral arm segments. M63 is part of the ], a group of galaxies that also includes ] (the 'Whirlpool Galaxy'). M63 is an ] with a ] nucleus.<ref>{{cite simbad|title=M 63|accessdate=16 November 2015}}</ref> The existence of a ] (SMBH) at the nucleus is uncertain; if it does exist, then the mass is estimated as {{Val|8.5e8|1.9|ul=solar mass}}.<ref name=Graham2008>{{citation | '''Messier 63''' (also known as '''M63''', '''NGC 5055''', or the '''Sunflower Galaxy''') is a ] in the ] ] consisting of a central disc surrounded by many short spiral arm segments. In the Catalogue of Named Galaxies, it is called '''Helianthus Canum Venaticorum''', after the Greek name for ''sunflower''.<ref>{{cite web|last1=Bodifee|first1=Gerard|title=Catalogue of One Thousand Named Galaxies|url=http://www.bodifee.be/wp-content/uploads/2015/08/2_CMG.pdf|accessdate=21 May 2017}}</ref> M63 is part of the ], a group of galaxies that also includes ] (the 'Whirlpool Galaxy'). M63 is an ] with a ] nucleus.<ref>{{cite simbad|title=M 63|accessdate=16 November 2015}}</ref> The existence of a ] (SMBH) at the nucleus is uncertain; if it does exist, then the mass is estimated as {{Val|8.5e8|1.9|ul=solar mass}}.<ref name=Graham2008>{{citation | ||
| title=Populating the Galaxy Velocity Dispersion - Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values | | title=Populating the Galaxy Velocity Dispersion - Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values | ||
| last1=Graham | first1=Alister W. | postscript=. | | last1=Graham | first1=Alister W. | postscript=. |
Revision as of 00:10, 29 July 2017
Messier 63 | |
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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. In the Catalogue of Named Galaxies, it is called Helianthus Canum Venaticorum, after the Greek name for sunflower. 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
- Bodifee, Gerard. "Catalogue of One Thousand Named Galaxies" (PDF). Retrieved 21 May 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, 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
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