Top Qs
Timeline
Chat
Perspective

NGC 4536

Spiral galaxy in the constellation Virgo From Wikipedia, the free encyclopedia

NGC 4536
Remove ads

NGC 4536 is an intermediate spiral galaxy in the constellation Virgo. It was discovered by German-British astronomer William Herschel on 24 January 1784.[7]

Quick facts Observation data (J2000 epoch), Constellation ...

NGC 4536 is located about 10° south of the midpoint of the Virgo Cluster. However, it is not considered a member of the cluster.[6] Rather, it is a member of the M61 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.[8][9][10] The morphological classification in the De Vaucouleurs system is SAB(rs)bc, which indicates it is a weakly barred spiral galaxy with a hint of an inner ring structure plus moderate to loosely wound arms.[6] It does not have a classical bulge around the nucleus.[11]

NGC 4536 has the optical characteristics of an HII galaxy, which means it is undergoing a strong burst of star formation.[11] This is occurring prominently in the ring that surrounds the bar and nucleus.[12] Based upon the level of X-ray emission from the core, it may have a small supermassive black hole with 104–106 times the mass of the Sun.[11]

One supernova has been observed in NGC 4536: SN 1981B (type Ia, mag. 12.3) was discovered by Dmitry Tsvetkov on 2 March 1981, located 51 arcseconds to the northeast of the Galactic Center.[13][14] It reached a peak visual magnitude of 12 on March 8 before steadily fading from view over the next two months.[6]

Remove ads

See also

References

Loading related searches...

Wikiwand - on

Seamless Wikipedia browsing. On steroids.

Remove ads