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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) | Abstract: | As 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 | Services: | Forum | Review | PDF | Favorites |
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