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NGC 4606

From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Virgo
NGC 4606
SDSS image of NGC 4606.
Observation data (J2000epoch)
ConstellationVirgo
Right ascension12h 40m 57.5s[1]
Declination11° 54′ 44″[1]
Redshift0.005470[1]
Heliocentric radial velocity1640 km/s[1]
Distance53.3 Mly (16.35 Mpc)[1]
Group orclusterVirgo Cluster
Apparent magnitude (V)12.67[1]
Characteristics
TypeSa[1]
Size~51,400 ly (15.75 kpc) (estimated)[1]
Apparent size (V)3.2 x 1.6[1]
Other designations
CGCG 70-213, IRAS 12384+1211, MCG 2-32-174, PGC 42516, UGC 7839, VCC 1859[1]

NGC 4606 is aspiral galaxy located about 55 millionlight-years away[2] in theconstellation ofVirgo.[3] NGC 4606 was discovered by astronomerWilliam Herschel on March 15, 1784.[4] It has a disturbed stellar disk suggesting the actions of gravitational interactions.[5]NGC 4607 may be a possible companion of NGC 4606.[6] However, theirredshifts differ by about 600 km/s, making it unlikely that they are a gravitationally bound pair.[7] NGC 4606 is a member of theVirgo Cluster.[8]

See also

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References

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  1. ^abcdefghij"NASA/IPAC Extragalactic Database".Results for NGC 4606. Retrieved2017-09-30.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2017-09-30.
  3. ^Rojas, Sebastián García."Galaxy NGC 4606 - Barred Spiral Galaxy in Virgo Constellation · Deep Sky Objects Browser".DSO Browser. Archived fromthe original on 2017-10-01. Retrieved2017-09-30.
  4. ^"New General Catalog Objects: NGC 4600 - 4649".cseligman.com. Retrieved2017-09-30.
  5. ^Saviane, Ivo; Ivanov, Valentin D.; Borissova, Jordanka (2007-08-01).Groups of Galaxies in the Nearby Universe: Proceedings of the ESO Workshop held at Santiago de Chile, December 5 - 9, 2005. Springer Science & Business Media.ISBN 978-3-540-71173-5.
  6. ^Koopmann, Rebecca A.; Kenney, Jeffrey D. P. (2004)."Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies".The Astrophysical Journal.613 (2):866–885.arXiv:astro-ph/0406243.Bibcode:2004ApJ...613..866K.doi:10.1086/423191.ISSN 0004-637X.S2CID 17519217.
  7. ^Chung, Aeree; Gorkom, J. H. van; Kenney, Jeffrey D. P.; Crowl, Hugh; Vollmer, Bernd (2009)."VLA Imaging of Virgo Spirals in Atomic Gas (VIVA). I. The Atlas and the H I Properties".The Astronomical Journal.138 (6): 1741.Bibcode:2009AJ....138.1741C.doi:10.1088/0004-6256/138/6/1741.ISSN 1538-3881.
  8. ^"Detailed Object Classifications".ned.ipac.caltech.edu. Retrieved2017-09-30.

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