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NGC 4868

From Wikipedia, the free encyclopedia

NGC 4868
NGC4868 - SDSS DR14
Observation data
ConstellationCanes Venatici
Right ascension12h 59m 08s
Declination37° 18′ 37″
Distance213 Mly
Apparent magnitude (B)12.9
Characteristics
TypeSAb

NGC 4868 is a spiral galaxy located 213 million light-years away in the constellation Canes Venatici.[1] It was discovered by William Herschel on March 17, 1787.[2] A 2002 study suggests that a quasar may exist within NGC 4868.[3]

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See also

References

  1. ^ "NGC 4868 - Spiral Galaxy in Canes Venatici". TheSkyLive.com. Archived from the original on October 27, 2021.
  2. ^ "NGCIC". Archived from the original on 2013-07-18.
  3. ^ 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.
This page was last edited on 28 April 2024, at 03:38
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