New model atmospheres for chemically peculiar stars
As stars evolve, their surfaces may be altered by several different mechanisms. These introduce distinctly unusual chemical peculiarities in their atmospheres. Hydrogen-deficient stars and subdwarf B stars are examples of such objects. These stars present a challenge for constructing reliable models...
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Queen's University Belfast
2007
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.486036 |