NGC 7836

Last updated
NGC 7836
SDSS NGC 7836.jpeg
SDSS image of NGC 7836.
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 00h 08m 01.6s [1]
Declination 33° 04′ 15″ [1]
Redshift 0.016358 [1]
Heliocentric radial velocity 4904 km/s [1]
Distance 260  Mly (80  Mpc) [1]
Apparent magnitude  (V)14.4 [1]
Characteristics
Type Irr?, Sb [1]
Size~83,000  ly (25.5  kpc) (estimated) [1]
Apparent size  (V)0.9 x 0.5 [1]
Other designations
CGCG 498-79, CGCG 499-51, IRAS 00054+3247, KUG 0005+327, Mrk 336, NPM1G +32.0005, PGC 608, UGC 65 [1]

NGC 7836 is an irregular spiral galaxy located about 260 million light-years away in the constellation Andromeda. [2] [3] It was discovered by the astronomer Lewis Swift on September 20, 1885. [3]

Contents

NGC 7836 is a member of the NGC 7831 Group and is part of the Perseus–Pisces Supercluster. [4] [5] [3] [6]

See also

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References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 7836. Retrieved 2019-03-11.
  2. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-03-11.
  3. 1 2 3 "New General Catalog Objects: NGC 7800 – 7840". cseligman.com. Retrieved 2017-08-11.
  4. ↑ Vettolani, G.; Baiesi Pillastrini, G. C. (1987-03-01). "Alignments of galaxies in the Perseus supercluster". Astronomy and Astrophysics. 175: 9–14. Bibcode:1987A&A...175....9V. ISSN   0004-6361.
  5. ↑ Cabanela, J. E.; Aldering, G. (1998-09-01). "Galaxy Alignments in the Pisces-Perseus Supercluster Revisited". The Astronomical Journal. 116 (3): 1094–1117. Bibcode:1998AJ....116.1094C. doi: 10.1086/300484 . ISSN   0004-6256.
  6. ↑ Garcia, A. M. (1993-07-01). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode:1993A&AS..100...47G. ISSN   0365-0138.
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