Nuclear and dynamical evolution of stellar systems
A rapid binary evolution algorithm is produced that enables modelling of even the most complex binary systems. In addition to all aspects of the single star algorithm, features such as mass transfer, mass accretion, common-envelope evolution, collisions, supernova kicks and angular momentum loss mec...
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University of Cambridge
2000
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.604827 |