Are Wolf-Rayet Stars Able to Pollute the Interstellar Medium of Galaxies? Results from Integral Field Spectroscopy

Figure 3

Oxygen abundance maps derived as described in the text and histogram distributions in linear scale for WR038, WR039, and WR057. In all images, each spaxel has 1^′′ resolution, north is up and east is left. The bars in the histogram represent spaxels with detected WR emission (red), spaxels in the same positions as the SDSS pointing (black), spaxels adjacent to this position (brown), and the other spaxels (grey). Same figure for WR266, WR404, and WR505.

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