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Pulsating white dwarfs and convection

Published online by Cambridge University Press:  09 October 2020

J. L. Provencal
Affiliation:
University of Delaware, Dept. of Physics and Astronomy, Newark, DE19716 email: jlp@udel.edu
M. H. Montgomery
Affiliation:
Dept. of Astronomy & University of Texas, Austin, TX email: mikemon@astro.as.utexas.edu
H. L. Shipman
Affiliation:
University of Delaware, Dept. of Physics and Astronomy, Newark, DE19716 email: jlp@udel.edu
The WET Team
Affiliation:
See www.physics.udel.edu/darc for a list of WET collaborators
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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.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

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