Chemical enrichment by Wolf-Rayet and Asymptotic Giant Branch Stars
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
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Dray_Chemical_enrichment_by_2003.pdf||3.17 MB||Adobe PDF||Request a copy|
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