NGC 5204

NGC 5204
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension13h 29m 36.5s
Declination+58° 25′ 07″
Redshift+201 km/s
Distance4.3-4.8 Mpc[1][2][3]
(14-14.5 million ly)
Apparent magnitude (V)11.73
Characteristics
TypeSA(s)m
Apparent size (V)5.0′ × 3.0'
Other designations
UGC 8490, PGC 47368, ZWG 294.39
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NCG 5204 is a Magellanic spiral galaxy located about 14.5 million light-years away from Earth[note 1] in the constellation of Ursa Major and is a member of the M101 Group of galaxies.[4][5] It has a galaxy morphological classification of SA(s)m and is highly irregular, with only the barest indication of any spiral arm structure.[3] The galaxy's most prominent feature is an extremely powerful X-ray source designated NGC 5204 X-1. This has resulted in the galaxy being the target of several studies due to the strength of the source and its relative proximity to Earth.[6][clarification needed]

  1. ^ Cite error: The named reference liuetal2004 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference zezas_2010 was invoked but never defined (see the help page).
  3. ^ a b Cite error: The named reference NED was invoked but never defined (see the help page).
  4. ^ P. Fouque; E. Gourgoulhon; P. Chamaraux; G. Paturel (1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement. 93: 211–233. Bibcode:1992A&AS...93..211F.
  5. ^ Vincent Sicotte; Claude Carignan & Daniel Durand (1996). "NGC 5204: A Strongly Warped Magellanic Spiral. I. Light Distribution and HII Kinematics". Astronomical Journal. 112: 1423–1428. Bibcode:1996AJ....112.1423S. doi:10.1086/118110.
  6. ^ T.P. Roberts; M.R. Goad; M.J.Ward; R.S.Warwick; et al. (2002). "The Nature Of Ultraluminous X-ray Sources In Nearby Galaxies". The Astrophysical Journal. 725 (1): 842–867. arXiv:1009.0525. Bibcode:2010ApJ...725..842L. doi:10.1088/0004-637X/725/1/842. S2CID 119112246.


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