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NGC 4305

From Wikipedia, the free encyclopedia
Dwarf spiral galaxy in the constellation Virgo
NGC 4305
SDSS image of NGC 4305.
Observation data (J2000epoch)
ConstellationVirgo
Right ascension12h 22m 03.6s[1]
Declination12° 44′ 27″[1]
Redshift0.006298[1]
Heliocentric radial velocity1888 km/s[1]
Distance98 Mly (30 Mpc)[1]
Apparent magnitude (V)13.4[1]
Characteristics
TypeSA(r)a[1]
Size~32,000 ly (9.7 kpc) (estimated)[1]
Apparent size (V)2.07 x 0.97[1]
Other designations
UGC 07432, VCC 0522, PGC 040030, MCG +02-32-013[1]

NGC 4305 is adwarf spiral galaxy[2] located about 100 millionlight-years away[3] in the constellationVirgo. The galaxy was discovered by astronomerJohn Herschel on May 2, 1829.[4] Although considered to be a member of theVirgo Cluster,[2][5] its high radial velocity and blue luminosity suggest it is in fact a background galaxy.[6] The galaxy has a nearby major companion;NGC 4306.[6]

NGC 4305 exhibits well-defined, smooth spiral arms which terminate well outside its central bulge.[7] This spiral structure appears to have been induced by a tidal interaction withNGC 4306.[8][9] Such a tidal interaction would also explain its deficiency inneutral hydrogen gas (HI).[6]

References

[edit]
  1. ^abcdefghij"NASA/IPAC Extragalactic Database".Results for NGC 4305. Retrieved2019-08-01.
  2. ^abDavidge, T. J. (2018-10-31)."The Stellar Contents of Intermediate Mass Disk Galaxies in the Virgo Cluster. I. GMOS Spectra".The Astronomical Journal.156 (5): 233.arXiv:1811.00041.Bibcode:2018AJ....156..233D.doi:10.3847/1538-3881/aae5fa.S2CID 119391307.
  3. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2019-08-02.
  4. ^"New General Catalog Objects: NGC 4300 - 4349".cseligman.com. Retrieved2019-08-02.
  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. ^abcSanchis, T.; Mamon, G. A.; Salvador-Sol´e, E.; Solanes, J. M. (2004-05-01)."The origin of H I-deficiency in galaxies on the outskirts of the Virgo cluster. II. Companions and uncertainties in distances and deficiencies".Astronomy and Astrophysics.418 (2):393–411.arXiv:astro-ph/0401367.Bibcode:2004A&A...418..393S.doi:10.1051/0004-6361:20034158.ISSN 0004-6361.
  7. ^"NGC 4305 - SA(s)a".The De Vaucouleurs Atlas of Galaxies. Retrieved2019-08-09.
  8. ^van den Bergh, Sidney; Pierce, Michael J.; Tully, R. Brent (1990-08-01). "Classification of galaxies on CCD frames".The Astrophysical Journal.359:4–14.Bibcode:1990ApJ...359....4V.doi:10.1086/169027.ISSN 0004-637X.
  9. ^Malin, D. (1994). "Interacting Galaxies in the Virgo Cluster".Astronomy from Wide-Field Imaging. Vol. 161. pp. 567–576.Bibcode:1994IAUS..161..567M.doi:10.1007/978-94-011-1146-1_119.ISBN 978-0-7923-2879-7.S2CID 118943109.

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