Fig. 1
Oxygen abundance vs. stellar mass for nearby dIrrs and BCDs. Filled blue and open magenta circles are data from Vaduvescu et al. (2007), and they represent BCDs and dIrrs, respectively; open magenta triangles are dIrrs observed by Lee et al. (2006), and the dashed line shows the best fit of their data. The solid line is the best linear fit of all the data.
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