Mode identification in slowly pulsating subdwarf-B stars from line-profile variations
In previous attempts to perform seismic modelling of pulsating subdwarf-B stars, various mode identification techniques have been used, with less success than in pulsating Main Sequence stars. In this work I investigate a method so far neglected in sdB stars, that is, mode identification from the li...
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University of Oxford
2007
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.491972 |