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Chemical Properties of Star‐Forming Dwarf Galaxies

  • Authors: Ovidiu Vaduvescu, Marshall L. McCall, and Michael G. Richer

Vaduvescu, McCall, & Richer 2007 The Astronomical Journal 134 604.

  • Provider: AAS Journals

Caption: Fig. 7.

Oxygen abundance vs. absolute sech magnitudes in ﹩K_{s}﹩ for dIs and BCDs. The dIs are plotted as circles, while BCDs are plotted as triangles. ﹩T_{e}﹩‐based abundances are plotted as filled symbols and ﹩R_{23}﹩‐based abundances as open symbols. The five outliers from Figs. 5 and 6 are not shown. The solid line represents the LZ relation for the dIs.

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