Asteroseismology from the main sequence to giant stars
The thesis focuses on the use of asteroseismology to probe the structure of stellar sources. By observing pulsational variability, a detailed description of the interior of stars, and the determination of stellar parameters can be obtained. An extensive sample of bright K and M class giant stars wer...
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University of Birmingham
2010
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.515570 |