Chemical abundances of very young intermediate mass stars
On the main sequence, roughly 10-20% of A- and B-type stars display a wide range of chemical peculiarities in their photospheres. It is unknown when during stellar evolution these chemical peculiarities develop, and the mechanisms for the formation of some peculiarities are Dot fully understood. In...
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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.601478 |