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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. 5.

Oxygen abundance vs. absolute sech magnitude in ﹩K_{s}﹩ for dIs. ﹩T_{e}﹩‐based abundances are plotted as filled symbols and ﹩R_{23}﹩‐based abundances as open symbols. Errors in metallicities are shown as vertical bars. Typical errors for absolute magnitudes are ~0.1 mag. Four outliers are labeled in the plot. The geometric mean fit to other dIs is plotted as a dashed line.

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