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Discovery of an Unusual Dwarf Galaxy in the Outskirts of the Milky Way

We announce the discovery of a new dwarf galaxy, Leo T, in the Local Group. It was found as a stellar overdensity in the Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The color-magnitude diagram of Leo T shows two well-defined features, which we interpret as a red giant branch and a sequence o...

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Published in:The Astrophysical journal 2007-02, Vol.656 (1), p.L13-L16
Main Authors: Irwin, M. J, Belokurov, V, Evans, N. W, Ryan-Weber, E. V, de Jong, J. T. A, Koposov, S, Zucker, D. B, Hodgkin, S. T, Gilmore, G, Prema, P, Hebb, L, Begum, A, Fellhauer, M, Hewett, P. C, Kennicutt, Jr., R. C, Wilkinson, M. I, Bramich, D. M, Vidrih, S, Rix, H.-W, Beers, T. C, Barentine, J. C, Brewington, H, Harvanek, M, Krzesinski, J, Long, D, Nitta, A, Snedden, S. A
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Language:English
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Summary:We announce the discovery of a new dwarf galaxy, Leo T, in the Local Group. It was found as a stellar overdensity in the Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The color-magnitude diagram of Leo T shows two well-defined features, which we interpret as a red giant branch and a sequence of young, massive stars. As judged from fits to the color-magnitude diagram, it lies at a distance of 420 kpc and has an intermediate-age stellar population with a metallicity of [Fe/H] = -1.6, together with a young population of blue stars of age 200 Myr. There is a compact cloud of neutral hydrogen with mass 10 super(5) M sub( )and radial velocity +35 km s super(-1) coincident with the object visible in the HIPASS channel maps. Leo T is the smallest, lowest luminosity galaxy found to date with recent star formation. It appears to be a transition object similar to, but much lower luminosity than, the Phoenix dwarf.
ISSN:1538-4357
0004-637X
1538-4357
DOI:10.1086/512183