DDO 169 explained

DDO 169
Epoch:J2000
Constellation Name:Canes Venatici
Z:+260 km/s
Dist Ly:6.03 / 8.23 Mpc[1] [2]
(19.7 / 26.8 million ly)
Type:IAm
Appmag V:14.61
Size V:2.7′ × 0.9'
Names:UGC 8331, PGC 46127

DDO 169 (also known as 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 × 1.5 kiloparsecs (16,000 × 5,000 lightyears). 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. The exact distance to the galaxy is not known, although a 1998 paper estimated the distance as 8.23 megaparsecs.

Notes and References

  1. Web site: NED results for UGC 8331. NED via University of California. 2009-03-08.
  2. Web site: Distances to five resolved galaxies in the Canes Venatici cloud . I.D. Karachentsev . I.O. Drovdozsky . July 1998 . Astronomy and Astrophysics Supplement Series . 2009-03-08 .
  3. 0901.4222. The rotation curves shapes of late-type dwarf galaxies. R.A. Swaters . R. Sancisi . T.S. van Albada . J.M. van der Hulst . 2009-01-27. Astronomy and Astrophysics. 10.1051/0004-6361:200810516 . 2009A&A...493..871S. 493. 3. 871–892. 14143255.