Are Wolf-Rayet Stars Able to Pollute the Interstellar Medium of Galaxies? Results from Integral Field Spectroscopy
Figure 1
Extinction corrected Hα maps of the six observed WR galaxies. In all images, each spaxel has of resolution. North is up, and east is to the left. Fluxes are in units of erg/s/cm2. The relative size in parsecs, at the adopted distance of each object, is indicated. For WR038, the spaxels where the WR bump was detected from our PMAS data are marked with red crosses.
