Chemical enrichment by Wolf-Rayet and Asymptotic Giant Branch Stars
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Dray, L M
Tout, Christopher A
Karakas, Amanda
Lattanzio, John
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Blackwell Publishing Ltd
Abstract
We present theoretical models of Wolf-Rayet (WR) stars for two different sets of mass-loss rates. We compare with observed properties of WR stars and discuss implications for the enrichment of the interstellar medium in both cases. Sets of stellar yields
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Monthly Notices of the Royal Astronomical Society
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Restricted until
2037-12-31
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