Other
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1817g&link_type=abstract
IUE Proposal ID #WRGCG
Other
Scientific paper
We are proposing to continue the investigation of continuum flux distributions of Wolf-Rayet stars from IUE and ground-based scanner observations. Wolf-Rayet stars make a major contribution to the overall luminosity and chemical enrichment of the galaxy', and have the largest mass loss rates of any known stars. However the mechanism driving their wind is not understood, and the variations observed in mass, luminosity and line strength within the same spectral subtypes lead one to question the evolutionary significance of these types. Initially, we hoped to derive effective temperatures and radii from the energy distribution and then sort out the other parameters. Instead, we found that reddening, possibly circumstellar, prevented this. We want to circumvent the reddening problem by observing W-R stars in the Large Magellanic Cloud, where the interstellar reddening is low, and differences from star to star may tell us primarily about circumstellar extinction and continua shapes. The brighter W-R stars in the LMC have already been observed with IUE, but the discovery by Massey and Conti that there is a three mag. spread in the absolute magnitudes of the single WN stars requires observation of some fainter stars. We also want to consider the relation between the continua and the radio mass loss. Only half of the stars with radio observations have IUE data, which is vital for providing wind terminal velocities. Additional observations of fainter W-R stars are necessary to insure that the radio mass loss rates which all lie in a very narrow range, do not suffer from a selection effect.
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