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- W3100018733 abstract "We demonstrate how pulsating white dwarfs can be used as an astrophysical laboratory for empirically constraining convection in these stars. We do this using a technique for fitting observed non-sinusoidal light curves, which allows us to recover the thermal response timescale of the convection zone (its “depth”) as well as how this timescale changes as a function of effective temperature. We also obtain mode identifications for the pulsation modes, allowing us to use asteroseismology to study the interior structure of these stars." @default.
- W3100018733 created "2020-11-23" @default.
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- W3100018733 date "2006-09-01" @default.
- W3100018733 modified "2023-09-23" @default.
- W3100018733 title "Mapping Convection Using Pulsating White Dwarf Stars" @default.
- W3100018733 hasPublicationYear "2006" @default.
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