NGC 4892 is a spiral[2][3][4] or lenticular galaxy[2] with LINER activity[4] located 275 million light-years away[5] in the constellation Coma Berenices.[6] It was discovered by the astronomer William Herschel on April 11, 1785,[6] and is a member of the Coma Cluster.[7]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4892. Retrieved November 10, 2018.
  2. ^ a b c "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved November 10, 2018.
  3. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved November 10, 2018.
  4. ^ a b "NGC 4892". Retrieved November 10, 2018.
  5. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved October 31, 2018.
  6. ^ a b "New General Catalog Objects: NGC 4850 - 4899". cseligman.com. Retrieved November 11, 2018.
  7. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved November 11, 2018.
    - "NGC 4892". Retrieved November 11, 2018.


Allikas: https://en.wikipedia.org/wiki/NGC_4892
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