UGCA 86 explained

UGCA 86
Epoch:J2000
Ra:[1]
Constellation Name:Camelopardalis
Z:67 ± 4 km/s
Dist Ly:[2]
Type:Im
Appmag V:13.5
Absmag V:-17.0
Size V:5.0 × 3.0
Names:PGC 14241

UGCA 86 is a Magellanic spiral galaxy. It was first thought to be part of the Local Group, but after the brightest stars in the galaxy were observed, it became clear that it was located in the IC 342/Maffei Group.[3] UGCA 86 is thought to be a satellite galaxy of IC 342, however the separation between the two galaxies is over 50% larger than the distance between the Milky Way and the Magellanic Clouds.[4]

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for UGCA 86 . 2006-11-30.
  2. 10.1051/0004-6361/202037993. KKH 22, the first dwarf spheroidal satellite of IC 342. 2020. Karachentsev. Igor D.. Makarova. Lidia N.. Brent Tully. R.. Anand. Gagandeep S.. Rizzi. Luca. Shaya. Edward J.. Afanasiev. Viktor L.. 218538458. Astronomy & Astrophysics. 638. A111. 2005.03132. 2020A&A...638A.111K.
  3. I. D. Karachentsev . The Local Group and Other Neighboring Galaxy Groups . Astronomical Journal . 2005 . 129 . 1 . 178–188 . 2005AJ....129..178K . 10.1086/426368. astro-ph/0410065 . 119385141 .
  4. H I Distribution and Kinematics of UGCA 86. Stil, J. M.. Gray, A. D.. Harnett, J. I.. 6461207. The Astrophysical Journal. 625. 1. 130–142. 2005. 2005ApJ...625..130S. 10.1086/424962. astro-ph/0408134.