NGC 4492
J2000 epoch) | |
---|---|
Constellation | Virgo |
Right ascension | 12h 30m 59.7s[1] |
Declination | 08° 04′ 40″[1] |
Redshift | 0.005804/1740 km/s[1] |
Distance | 90,950,000 ly[2][3] |
Apparent magnitude (V) | 13.0[1] |
Characteristics | |
Type | SA(s)a?[1] |
Size | ~33,450 ly (estimated)[1] |
Apparent size (V) | 1.58 x 1.25[1] |
Other designations | |
IC 3438, PGC 41383, UGC 7656, VCC 1330[1] |
NGC 4492 is a
Arnold Schwassmann on January 23, 1900, and was listed as IC 3438.[6] NGC 4492 lies in the direction of the Virgo Cluster. However, it is not considered to be a member of that cluster.[7]
Physical characteristics
NGC 4492 has a relatively large
Interstellar dust.[8]
Virgo Cluster membership
NGC 4492 is listed in the Virgo Cluster Catalog as VCC 1330.[8] However, distance estimates to the galaxy place it at a location far outside of the cluster's center.[2][7] Also, its radial velocity indicates that NGC 4492 is not gravitationally bound to the Virgo Cluster but is expanding away from it. Therefore, NGC 4492 is not a member of the Virgo Cluster but rather a background galaxy.[7]
See also
References
- ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 4492. Retrieved 2017-10-25.
- ^ S2CID 15207214.
- ^ "parsecs to lightyears conversion". Retrieved 2017-09-30.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-10-27.
- ^ Rojas, Sebastián García. "Galaxy NGC 4492 - Spiral Galaxy in Virgo Constellation · Deep Sky Objects Browser". DSO Browser. Retrieved 2017-10-27.
- ^ "New General Catalog Objects: NGC 4450 - 4499". cseligman.com. Retrieved 2017-10-27.
- ^ S2CID 18787428.
- ^ doi:10.1086/113874.
External links
Wikimedia Commons has media related to NGC 4492.
- NGC 4492 on