| 词条 | UGCA 86 |
| 释义 |
| name = UGCA 86 | image = File:UGCA 86 color cutout hst 9771 14 acs wfc f814w f606w sci.jpg | caption = UGCA 86 as taken by Hubble Space Telescope | epoch = J2000 | ra = {{RA|03|59|50.5}}[1] | dec = {{DEC|+67|08|37}}[1] | constellation name = Camelopardalis | z = 67 ± 4 km/s[1] | dist_ly ={{convert|2600000|pc|ly|abbr=on|lk=on|order=flip}}[4] | type = Im[1] | appmag_v = 13.5[1] | absmag_v = -17.0[4] | size_v = 5′.0 × 3′.0 [1] | notes = | names = PGC 14241[1] }}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.[2] 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.[3] References1. ^1 2 3 4 5 6 {{cite web | title=NASA/IPAC Extragalactic Database | work=Results for UGCA 86 | url=http://nedwww.ipac.caltech.edu/ | accessdate=2006-11-30}} 2. ^{{cite journal | author=I. D. Karachentsev | title=The Local Group and Other Neighboring Galaxy Groups | journal=Astronomical Journal | year=2005 | volume=129 | issue=1 | pages=178–188 | bibcode=2005AJ....129..178K | doi=10.1086/426368|arxiv = astro-ph/0410065 }} 3. ^1 2 {{cite journal|title=H I Distribution and Kinematics of UGCA 86|author1=Stil, J. M.|author2=Gray, A. D.|author3=Harnett, J. I.|journal=The Astrophysical Journal|volume=625|issue=1|pages=130–142|date=2005|bibcode=2005ApJ...625..130S|doi=10.1086/424962|arxiv=astro-ph/0408134}} External links
4 : Irregular galaxies|IC 342/Maffei Group|Principal Galaxies Catalogue objects|UGCA objects |
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