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25 April 2024
 
  » arxiv » arxiv.0705.1378

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A Pair of Bootes: A New Milky Way Satellite
S.M. Walsh ; H. Jerjen ; B. Willman ;
Date 10 May 2007
Subject Astrophysics (astro-ph)
AbstractAs part of preparations for a southern sky search for faint Milky Way dwarf galaxy satellites, we report the discovery of a stellar overdensity in the Sloan Digital Sky Survey Data Release 5, lying at an angular distance of only 1.5 degrees from the recently discovered Bo{"o}tes dwarf. The overdensity was detected well above statistical noise by employing a sophisticated data mining algorithm and does not correspond to any catalogued object. Overlaid isochrones using stellar population synthesis models show that the color-magnitude diagram of that region has the signature of an old (12 Gyr), metal-poor (${ m Fe/H}approx-2.0$) stellar population at a tentative distance of 60 kpc, evidently the same heliocentric distance as the Bo"otes dwarf. We estimate the new object to have a total magnitude of $M_{V}sim-3.1pm1.1$ mag and a half-light radius of $r_{h}=4’.1pm1’.6$ ($72pm28$ pc) placing it in an apparent $40<r_{h}<100$ pc void between globular clusters and dwarf galaxies, occupied only by another recently discovered Milky Way Satellite, Coma Berenices.
Source arXiv, arxiv.0705.1378
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