Observational constraints on pre-main sequence stellar evolution from time-series analysis of open cluster stars
Observational constraints on evolutionary models of low-mass stars (≲ 1.0 M<sub>⊙</sub>) are presently extremely scarce on the pre-main sequence. Recent observational evidence has indicated substantial discrepancies between the predictions of these models and observations made in binary...
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University of Cambridge
2007
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.604961 |