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.
Supernova One supernova has been observed in MCG +07-33-027.
SN 2005bk (Type Ic, mag. 18) was discovered by R. A. Jansen, K. Tamura, and N. A. Grogin on April 2, 2005.
See also NGC 3034 Baby Boom Galaxy Morphological Catalogue of Galaxies
References
External links MCG +07-33-027 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


