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- W1520205276 abstract "As it is long known, the presence of a convective region creates a discontinuity in the chemical profile of a star, which in turn translates into a sharp variation of the adiabatic sound speed. This variation produces an oscillatory behavior of the pulsation frequencies, to which low degree p-modes are sensitive. We investigate the possibility of detecting the signature related to the presence of a convective core in the frequency spectrum of low-mass stars by means of suitable frequency combinations (such as separations and ratios)" @default.
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- W1520205276 date "2010-04-16" @default.
- W1520205276 modified "2023-09-26" @default.
- W1520205276 title "Convective core size determination using asteroseismic data" @default.
- W1520205276 cites W3102300107 @default.
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- W1520205276 doi "https://doi.org/10.48550/arxiv.1004.2928" @default.
- W1520205276 hasPublicationYear "2010" @default.
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