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- W37605130 abstract "Abstract We briefly present a method to perform detailed asteroseismological analyses of pulsating subdwarf B (sdB) stars (also referred to as the EC14026 stars). We use a forward approach based on the computation of large grids of sdB stellar models (each model being analyzed with a linear nonadiabatic pulsation code) to derive, in an objective way, the most appropriate set of model parameters that can best reproduce the observed period spectrum of a given sdB pulsator. We discuss an illustrative application of this method to the pulsating sdB star PG 1047+003, for which we derive the fundamental parameters T eff , log g , M tot , and M env ." @default.
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- W37605130 date "2002-01-01" @default.
- W37605130 modified "2023-10-10" @default.
- W37605130 title "Asteroseismic Analysis of Pulsating Subdwarf B Stars" @default.
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- W37605130 doi "https://doi.org/10.1017/s0252921100016511" @default.
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