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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University of Cambridge
2003
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Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.598644 |