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- W2293856596 abstract "Recent determinations of the internal composition and structure of two helium-atmosphere variable white dwarf stars, GD 358 and CBS 114, have led to conflicting implied rates for the 12C(α,γ)16O reaction. If we assume that both stars were formed through single-star evolution, then the initial analyses of their pulsation frequencies must have differed in some systematic way. I present improved fits to the two sets of pulsation data, helping to resolve the tension between the initial results." @default.
- W2293856596 created "2016-06-24" @default.
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- W2293856596 date "2003-01-01" @default.
- W2293856596 modified "2023-09-23" @default.
- W2293856596 title "White Dwarf Seismology and the 12C(α,γ)16O Rate" @default.
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- W2293856596 doi "https://doi.org/10.1007/978-94-010-0215-8_75" @default.
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