Stellar pulsation and the RV Tauri phenomenon
On the basis of observational data it is argued that RV Tauri variables, and probably yellow semiregular (SRd) variables, are closely related in every way to type II cepheid stars. Assuming that a single mass (~O.6 M~) is applicable to all three classes of star linear, nonadiabatic pulsation models...
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University of St Andrews
1985
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.571490 |