Mass-loss properties of the most massive stars in 30 Doradus
Our understanding of high-mass star evolution is tightly connected to our understanding of their mass-loss properties. The initial and final mass are significantly different as a result of mass loss. Massive stars have strong stellar winds and high ionising fluxes and are the main sources for mechan...
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Queen's University Belfast
2013
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.602438 |