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29 April 2024
 
  » arxiv » astro-ph/0606633

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A Curious New Milky Way Satellite in Ursa Major
D.B. Zucker ; V. Belokurov ; N.W. Evans ; J.T. Kleyna ; M.J. Irwin ; M.I. Wilkinson ; M. Fellhauer ; D.M. Bramich ; G. Gilmore ; H.J. Newberg ; B. Yanny ; J.A. Smith ; P.C. Hewett ; E.F. Bell ; H.-W. Rix ; O.Y. Gnedin ; S. Vidrih ; R.F.G. Wyse ; B. Willman ; E.K. Grebel ; D.P. Schneider ; T.C. Beers ; A.Y. Kniazev ; J.C. Barentine ; H. Brewington ; J. Brinkmann ; M. Harvanek ; S.J. Kleinman ; J. Krzesinski ; D. Long ; A. Nitta ; S.A. Snedden ;
Date 4 Jul 2006
AbstractIn this Letter, we study a localized stellar overdensity in the constellation of Ursa Major, first identified in Sloan Digital Sky Survey (SDSS) data and subsequently followed up with Subaru imaging. Its color-magnitude diagram (CMD) shows a well-defined sub-giant branch, main sequence and turn-off, from which we estimate a distance of ~30 kpc and a projected size of ~250 x 125 pc. The CMD suggests a composite population with some range in metallicity and/or age. Based on its extent and stellar population, we argue that this is a previously unknown satellite galaxy of the Milky Way, hereby named Ursa Major II (UMa II) after its constellation. Using SDSS data, we find an absolute magnitude of M_V ~ -3.8, which would make it the faintest known satellite galaxy. UMa II’s isophotes are irregular and distorted with evidence for multiple concentrations; this suggests that the satellite is in the process of disruption.
Source arXiv, astro-ph/0606633
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