Measuring Rotation Rates and Magnetic Fields of Wolf-Rayet Stars

Details Measuring Rotation Rates and Magnetic Fields of Wolf-Rayet Stars Measuring Rotation Rates and Magnetic Fields of Wolf-Rayet Stars

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388...79s&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

2

Scientific paper

Although our knowledge of the descendants of the most massive O stars, WR stars, has greatly improved in the last few decades, there are still a few physical parameters for which we have only very little information. In this paper, we present preliminary results of a project aimed at measuring two of these, namely rotation rates and magnetic fields, for a sample of WR stars.

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