UGC 8331

UGC 8331
Observation data (J2000 epoch)
Constellation Canes Venatici
Right ascension 13h 15m 30.31s
Declination +47° 29′ 56.2″
Redshift +260 km/s
Distance 6.03 / 8.23 Mpc[1][2]
(19.7 / 26.8 million ly)
Type IAm
Apparent dimensions (V) 2.7′ × 0.9'
Apparent magnitude (V) 14.61
Other designations
DDO 169, PGC 46127
See also: Galaxy, List of galaxies

UGC 8331 is an irregular galaxy located in the constellation Canes Venatici. It is a member of the M51 Group of galaxies and measures approximately 5 x 1.5 kiloparsecs (16,000 x 5,000 lightyears).[1] The galaxy's large-scale structure is very unorganized and it has two clusters of stars in its outer portions in addition to the cluster in the center.[3] These clusters make it practically impossible to determine the galaxy's rotation curve and contributes to a large variation in distance figures that are derived with different methods.[1][3] The exact distance to the galaxy is not known, although a 1998 paper estimated the distance as 8.23 megaparsecs.[2]

References

  1. ^ a b c "NED results for UGC 8331". NED via University of California. http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=UGC+8331&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES. Retrieved 2009-03-08. 
  2. ^ a b I.D. Karachentsev, I.O. Drovdozsky (1998-07). "Distances to five resolved galaxies in the Canes Venatici cloud". Astronomy and Astrophysics Supplement Series. http://aas.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aas/pdf/1998/13/ds7328.pdf. Retrieved 2009-03-08. 
  3. ^ a b R.A. Swaters, R. Sancisi, T.S. van Albada, J.M. van der Hulst (2009-01-27). "The rotation curves shapes of late-type dwarf galaxies". Astronomy and Astrophysics. arXiv:0901.4222. Bibcode 2009A&A...493..871S. doi:10.1051/0004-6361:200810516.