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- W2012809691 abstract "The pulsational stability of massive, chemically homogeneous stars of Population I has been investigated for a range of simple opacity representations consisting of a straight sum of electron-scattering and modified Kramers opacity. The critical mass for stability against nuclear-energized pulsations is found to be extraordinarily sensitive to small changes in the coefficient and/or temperature exponent of the absorption part of the opacity law. A gradual increase in the atomic absorption (dominant near the stellar surface) first raises the critical mass, then restricts the upper mass limit for instability, and finally eliminates pulsational instability at all masses." @default.
- W2012809691 created "2016-06-24" @default.
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- W2012809691 date "1974-11-01" @default.
- W2012809691 modified "2023-09-27" @default.
- W2012809691 title "Influence of opacity on the pulsational stability of massive stars with uniform chemical composition. II - Modified Kramers opacity" @default.
- W2012809691 doi "https://doi.org/10.1086/153204" @default.
- W2012809691 hasPublicationYear "1974" @default.
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