Fig. 10.
Metallicity – baryonic (gas and stars) mass relation of SF dwarfs. The dashed line represents linear fit using 28 dIs from LV and Virgo (Vaduvescu et al. 2007). The few A1367 and Hercules objects confine quite well with this linear trend, probing the fundamental metallicity – mass relation for SF dwarfs. The cross in the upper left shows typical uncertainties in the two parameters.
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