NGC 4326

Barred spiral galaxy in the constellation of Virgo From Wikipedia, the free encyclopedia

NGC 4326 is a barred spiral galaxy with a ring[2] located about 330 million light-years away[3] in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784,[4] who described it as "vF, S, R, bM, 1st of 3".[5] It is a large galaxy, with a diameter of around 200,000 ly (61 kpc) making it nearly twice the size of the Milky Way.[3] NGC 4326 is also classified as a LINER galaxy.[6] Despite being listed in the Virgo Cluster catalog as VCC 623, it is not a member of the Virgo Cluster but instead a background galaxy.[7]

Quick facts Observation data (J2000 epoch), Constellation ...
NGC 4326
NGC 4326 imaged by the Vera C. Rubin Observatory
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 23m 11.6s[1]
Declination06° 04 20[1]
Redshift0.023756[1]
Heliocentric radial velocity7122 km/s[1]
Distance330 Mly (102 Mpc)[1]
Apparent magnitude (V)14.19[1]
Characteristics
TypeSAB(r)ab+[1]
Size~200,700 ly (61.54 kpc) (estimated)[1]
Apparent size (V)1.5 x 1.1[1]
Other designations
UGC 07454, VCC 0623, PGC 040192, MCG +01-32-033, CGCG 042-064[1]
Close

NGC 4326 is host to a supermassive black hole with and estimated mass of 3.7×108 solar masses.[8]

Nearby Galaxies

NGC 4326 forms a pair with the galaxy NGC 4333, known as [T2015] nest 102514,[9][10] in which NGC 4326 is the brightest member of the pair.[10] Both galaxies are part of the CfA2 Great Wall.[11]

See also

References

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