Figure 4 from MMT Extremely Metal-Poor Galaxy Survey. I. An Efficient Technique to Identify Metal-Poor Galaxies

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MMT Extremely Metal-Poor Galaxy Survey. I. An Efficient Technique to Identify Metal-Poor Galaxies

Authors: Warren R. Brown, Lisa J. Kewley, and Margaret J. Geller

BROWN, KEWLEY, & GELLER 2008 The Astronomical Journal 135 92.

Provider: AAS Journals

Caption: Figure 4.

Color–magnitude distribution of nearby BCGs (Gil de Paz et al. 2003) and our 11 metal-poor galaxies, for which we estimate ( B − R) from SDSS photometry (Fukugita et al. 1996).

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