Back to Volume
Paper: Measuring Rotation Rates and Magnetic Fields of Wolf-Rayet Stars
Volume: 388, Mass Loss from Stars and the Evolution of Stellar Clusters
Page: 79
Authors: St-Louis, N.; Chené, A.-N.; de la Chevrotière, A.; Moffat, A.F.J.
Abstract: 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.
Back to Volume