NGC 4536 | |
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![]() NGC 4536 imaged by the Mount Lemmon Skycenter | |
Observation data (J2000 epoch) | |
Constellation | Virgo |
Right ascension | 12h 34m 27.129s [1] |
Declination | +02° 11′ 16.37″ [1] |
Redshift | 0.006031 ± 0.000003 [2] |
Heliocentric radial velocity | 1808 ± 1 [3] km/s |
Distance | 48.7 ± 0.9 Mly (14.9 ± 0.3 Mpc) [4] |
Apparent magnitude (V) | 11.1 [5] |
Characteristics | |
Type | SAB(rs)bc [6] |
Size | ~108,200 ly (33.17 kpc) (estimated) [5] |
Apparent size (V) | 7.6′ × 3.2′ [5] |
Other designations | |
UGC 7732, MCG +00-32-023, PGC 41823, CGCG 014-068 [5] |
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]
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]