MCG +07-33-027 | |
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Starburst galaxy MCG +07-33-027 as imaged by the Hubble Space Telescope. | |
Observation data (J2000 epoch) | |
Constellation | Hercules |
Right ascension | 16 02 16.6 |
Declination | 42° 55′ 01″ |
Redshift | 0.024486/7341 km/s |
Distance | 329,462,000 ly |
Apparent magnitude (V) | 14.5 |
Characteristics | |
Type | Sa |
Size | ~104,057.8 ly (estimated) |
Apparent size (V) | 0.86' x 0.74 |
Other designations | |
PGC 56779 |
MCG +07-33-027 is an isolated spiral galaxy located about 330 million light-years away in the constellation Hercules. It has a very high rate of star formation which would make it a starburst galaxy. Normally, starburst galaxies are triggered by the collision of another galaxy. However most galaxies are in groups or clusters, while MCG +07-33-027 is solitary. Therefore, the cause of the starburst was not due to a collision or by the passing of a nearby galaxy and so the cause of the activity remains unknown.
On April 2, 2005, SN 2005bk, a supernova (type Ic, mag. 18) was discovered in MCG +07-33-027.
See also
References
- ^ "NASA/IPAC Extragalactic Database". Results for MCG +07-33-027. Retrieved 2017-07-26.
- ^ "A lonely birthplace". www.spacetelescope.org. Retrieved 2017-07-27.
- "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-07-27.
- "Principal Galaxy Catalog (PGC) Objects 56500 to 56999". cseligman.com. Retrieved 2017-07-27.
- "IAUC 8512: 2005bk; 2005bl; 9P". www.cbat.eps.harvard.edu. Retrieved 2017-07-27.
- Transient Name Server entry for SN 2005bk. Retrieved 3 August 2024.
External links
- MCG +07-33-027 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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