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Pulsating white dwarfs and convection
Published online by Cambridge University Press: 09 October 2020
Abstract
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Convection is a highly turbulent, three dimensional process that is traditionally treated using a simple, local, time independent description. Convection is one of the largest sources of theoretical uncertainty in stellar modeling. We outline recent progress in studies using pulsating white dwarfs to constrain convection and calibrate mixing length theory.
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- © International Astronomical Union 2020
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