Jump to content

NGC 4595

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Loooke (talk | contribs) at 16:37, 4 February 2021 (removed Category:Spiral galaxies; added Category:Intermediate spiral galaxies using HotCat). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

NGC 4595
Sloan Digital Sky Survey image of NGC 4595.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 39m 51.9s[1]
Declination15° 17′ 52″[1]
Redshift0.002105[1]
Heliocentric radial velocity631 km/s[1]
Distance42 Mly (13 Mpc)[1]
Group or clusterVirgo Cluster
Apparent magnitude (V)12.91[1]
Characteristics
TypeSAB(rs)b[1]
Size~23,600 ly (7.23 kpc) (estimated)[1]
Apparent size (V)1.7 x 1.1[1]
Other designations
CGCG 99-106, IRAS 12373+1534, MCG 3-32-81, PGC 42396, UGC 7826, VCC 1811[1]

NGC 4595 is a spiral galaxy located about 42 million light-years away[2] in the constellation Coma Berenices.[3] NGC 4595 was discovered by astronomer William Herschel on January 14, 1787.[4] NGC 4595 is a member of the Virgo Cluster.[5][6]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4595. Retrieved 2018-03-08.
  2. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-03-08.
  3. ^ "Revised NGC Data for NGC 4595". spider.seds.org. Retrieved 2018-03-08.
  4. ^ "New General Catalog Objects: NGC 4550 - 4599". cseligman.com. Retrieved 2018-03-08.
  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. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-03-08.

External links