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NGC 4586

From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Virgo
NGC 4586
SDSS image of NGC 4586.
Observation data (J2000epoch)
ConstellationVirgo
Right ascension12h 38m 28.4s[1]
Declination04° 19′ 09″[1]
Redshift0.002648[1]
Heliocentric radial velocity794 km/s[1]
Distance51 Mly (15.5 Mpc)[1]
Group orclusterVirgo II Groups
Apparent magnitude (V)12.7[1]
Characteristics
TypeSA(s)a[1]
Size~60,900 ly (18.68 kpc) (estimated)[1]
Apparent size (V)2.90 x 0.99[1]
Other designations
CGCG 42-187, IRAS 12359+0435, MCG 1-32-122, PGC 42241, UGC 7804, VCC 1760[1]

NGC 4586 is aspiral galaxy located about 50 millionlight-years away[2] in the constellationVirgo.[3] The galaxy was discovered by astronomerWilliam Herschel on February 2, 1786.[4] Although listed in the Virgo Cluster Catalog,[5] NGC 4586 is considered to be a member of theVirgo II Groups which form a southern extension of theVirgo cluster.[6][7] NGC 4586 is currently in the process of infalling into theVirgo Cluster and is predicted to enter the cluster in about 500 million years.[8]

Boxy/Peanut bulge

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NGC 4586 has a boxy or peanut-shaped bulge. The bulge has been interpreted to be a bar viewed edge-on.[9][10]

See also

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References

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  1. ^abcdefghij"NASA/IPAC Extragalactic Database".Results for NGC 4586. Retrieved2018-03-02.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2018-03-03.
  3. ^"Revised NGC Data for NGC 4586".spider.seds.org. Retrieved2018-03-03.
  4. ^"New General Catalog Objects: NGC 4550 - 4599".cseligman.com. Retrieved2018-03-03.
  5. ^Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area".The Astronomical Journal.90:1681–1759.Bibcode:1985AJ.....90.1681B.doi:10.1086/113874.ISSN 0004-6256.
  6. ^Tully, R. B. (June 1982)."The Local Supercluster".The Astrophysical Journal.257:389–422.Bibcode:1982ApJ...257..389T.doi:10.1086/159999.ISSN 0004-637X.
  7. ^"The Virgo II Groups".www.atlasoftheuniverse.com. Retrieved2018-03-03.
  8. ^Tully, R. B.; Shaya, E. J. (June 1984)."Infall of galaxies into the Virgo cluster and some cosmological constraints".The Astrophysical Journal.281:31–55.Bibcode:1984ApJ...281...31T.doi:10.1086/162073.ISSN 0004-637X.
  9. ^Corsini, E. M.; Pizzella, A.; Coccato, L.; Bertola, F. (2003-09-01). "Minor-axis velocity gradients in spirals and the case of inner polar disks".Astronomy & Astrophysics.408 (3):873–885.arXiv:astro-ph/0306382.Bibcode:2003A&A...408..873C.doi:10.1051/0004-6361:20030951.ISSN 0004-6361.S2CID 17961897.
  10. ^Bender, Ralf (2003-01-23).The Mass of Galaxies at Low and High Redshift: Proceedings of the European Southern Observatory and Universitäts-Sternwarte München Workshop Held in Venice, Italy, 24-26 October 2001. Springer Science & Business Media.ISBN 9783540002055.

External links

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