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- W1617956899 abstract "It is shown that in presence of URCA shell pulsational energy losses due to neutrino emission and nonequilibrium beta heating are much less than energy losses by excitation of short-wavelength acoustic waves. Convective motion in presence of URCA shell is considered, and equations generalizing the mean free path model of convection are derived." @default.
- W1617956899 created "2016-06-24" @default.
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- W1617956899 date "2000-04-19" @default.
- W1617956899 modified "2023-09-25" @default.
- W1617956899 title "Oscillations and convective motion in stars with URCA shells" @default.
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- W1617956899 doi "https://doi.org/10.48550/arxiv.astro-ph/0004281" @default.
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