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NGC 4868

From Wikipedia, the free encyclopedia
Galaxy in the constellation Canes Venatici
NGC 4868
SDSS image of NGC 4868
Observation data (J2000 epoch)
Constellation Canes Venatici
Right ascension 12h 59m 08.88278s[1]
Declination +37° 18′ 37.4675″[1]
Redshift 0.015597[2]
Heliocentric radial velocity 4639 km/s[2]
Distance 241 Mly (74.0 Mpc)[3]
Apparent magnitude (B)12.95[4]
Characteristics
Type SAab?[5]
Apparent size (V)1.6′[3]
Other designations
UGC 8099, MCG +06-29-004, PGC 44557[2]

NGC 4868 is an unbarred spiral galaxy located about 240 million light-years away[3] in the constellation Canes Venatici.[6] It was discovered by William Herschel on March 17, 1787.[7] A 2002 study suggests that a quasar may exist within NGC 4868.[8]

See also

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References

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  1. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics . 649: A1. arXiv:2012.01533 . Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657 . S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e).
  2. ^ a b c "NGC 4868". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2024年10月26日.
  3. ^ a b c Maragkoudakis, A.; Zezas, A.; Ashby, M. L. N.; Willner, S. P. (2014). "Aperture effects on spectroscopic galaxy activity classification". Monthly Notices of the Royal Astronomical Society. 441 (3): 2296–2308. arXiv:1404.0620 . Bibcode:2014MNRAS.441.2296M. doi:10.1093/mnras/stu634 .
  4. ^ "Search specification: NGC 4868". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2024年10月26日.
  5. ^ "Results for object NGC 4868 (NGC 4868)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2024年10月26日.
  6. ^ "NGC 4868 - Spiral Galaxy in Canes Venatici". TheSkyLive.com. Archived from the original on October 27, 2021.
  7. ^ "NGCIC". Archived from the original on 2013年07月18日.
  8. ^ Burbidge, E. Margaret; Burbidge, Geoffrey; Arp, Halton C.; Zibetti, Stefano (2003). "QSOs Associated with M82". The Astrophysical Journal. 591 (2): 690–694. arXiv:astro-ph/0303625 . Bibcode:2003ApJ...591..690B. doi:10.1086/375411. S2CID 118875813.

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