Fig. A.1
Relation between te([O iii]) and total oxygen abundances (12 + lg(O/H)) for Hii galaxies from H06, H08 and H11 (solid circles), and Hii galaxies (open circles), GEHRs (upward triangles) and diffuse Hii regions in the Galaxy and the Magellanic Clouds (squares) from Pérez-Montero & Díaz (2005). The solid line is the actual fit to the data. The temperatures are in units of 104 K.
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