Models of White Dwarfs, Radial Pulsations and Vibrational Stability

Vauclair, G.

doi:10.1007/978-94-010-3081-6_21

G. Vauclair²

Part of the book series: International Astronomical Union/Union Astronomical International ((IAUS,volume 42))

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Abstract

We have computed a set of models of white dwarfs. The equation of state is the Chandrasekhar (1939) one corrected by Salpeter (1961). It takes into account both the interactions between particles and the effect of non-zero temperature.

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Institut d’Astrophysique de Paris, France
G. Vauclair

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G. Vauclair
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University of Minnesota, Minneapolis, Minn., USA
W. J. Luyten

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Vauclair, G. (1971). Models of White Dwarfs, Radial Pulsations and Vibrational Stability. In: Luyten, W.J. (eds) White Dwarfs. International Astronomical Union/Union Astronomical International, vol 42. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3081-6_21

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DOI: https://doi.org/10.1007/978-94-010-3081-6_21
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3083-0
Online ISBN: 978-94-010-3081-6
eBook Packages: Springer Book Archive

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