Pulsations in white dwarf stars
G. Fontaine, P. Bergeron, P. Brassard, S. Charpinet, P. Dufour, N. Giammichele, S. K. Randall, V. Van Grootel
Abstract
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G. Fontaine, P. Bergeron, P. Brassard, S. Charpinet, P. Dufour, N. Giammichele, S. K. Randall, V. Van Grootel
Abstract
Open-access reader
Abstract We first present a brief description of the six distinct families of pulsating white dwarfs that are now known. These are all opacity-driven pulsators showing low- to mid-order, low-degree gravity modes. We then discuss some recent highlights that have come up in the field of white dwarf asteroseismology.
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Abstract We first present a brief description of the six distinct families of pulsating white dwarfs that are now known. These are all opacity-driven pulsators showing low- to mid-order, low-degree gravity modes. We then discuss some recent highlights that have come up in the field of white dwarf asteroseismology.
Key concepts: Asteroseismology, White dwarf, Physics, Opacity, Stars, Astrophysics, White (mutation), Astronomy