Proceedings of the Workshop
"The Magellanic Clouds and Other Dwarf Galaxies"
of the Bonn/Bochum-Graduiertenkolleg

A photometric method to study the Wolf-Rayet content

of compact H II regions in nearby galaxies

P. Royer, J.-M. Vreux, and J. Manfroid

 [Fig. 1]
Fig. 1. Simulations for WN binaries performed in a color diagram allowing a discrimination between the WNEs, the WNEw and the late WN. Some discrimination exists also among the late WN but this is better achieved with other color indices (see Royer, Vreux & Manfroid 1998, RVM). The symbols are explained on the right. Some WR stars spectra have been ``mixed'' with an O5V spectra of various relative intensities as can happen in case of line of sight contamination
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First version: 25thJuly,1998
Last update: 30thSeptember,1998
Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)