Wolf-Rayet stars and chemical enrichment

Computational models of Wolf-Rayet and other massive stars are presented at solar metallicity and at a range of non-solar metallicities from Z = 0.03 to Z = 0.0001. The effects of differing mass-loss rates, evolutionary paths and initial mass distributions are quantified and the resulting Wolf-Rayet...

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Bibliographic Details
Main Author: Dray, L. M.
Published: University of Cambridge 2003
Subjects:
520
Online Access:http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.598644