Hydrogen burning on a white dwarf accreting hydrogen in a binary system

S. A. Glasner; G. Rakavy; Y. Tuchman

doi:10.1007/BF00652938

Hydrogen burning on a white dwarf accreting hydrogen in a binary system

S. A. Glasner^*
, G. Rakavy
, Y. Tuchman

^*Corresponding author for this work

Racah Institute of Physics

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

We follow the accretion of hydrogen-rich matter onto the surface of a white dwarf in a close binary system. Two phases of accretion are assumed. First-slow accretion from the interstellar clouds, second-fast accretion from the companion. Hydrogen is ignited at the interface between the fast and slowly accreted layers. After a short runaway burning continues in the form of quasistationary deflagration front propagating inwards. The features of this front are discussed. A possibility of mass loss is indicated.

Original language	English
Pages (from-to)	397-403
Number of pages	7
Journal	Astrophysics and Space Science
Volume	80
Issue number	2
DOIs	https://doi.org/10.1007/BF00652938
State	Published - Dec 1981

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abstract = "We follow the accretion of hydrogen-rich matter onto the surface of a white dwarf in a close binary system. Two phases of accretion are assumed. First-slow accretion from the interstellar clouds, second-fast accretion from the companion. Hydrogen is ignited at the interface between the fast and slowly accreted layers. After a short runaway burning continues in the form of quasistationary deflagration front propagating inwards. The features of this front are discussed. A possibility of mass loss is indicated.",

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AU - Rakavy, G.

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N2 - We follow the accretion of hydrogen-rich matter onto the surface of a white dwarf in a close binary system. Two phases of accretion are assumed. First-slow accretion from the interstellar clouds, second-fast accretion from the companion. Hydrogen is ignited at the interface between the fast and slowly accreted layers. After a short runaway burning continues in the form of quasistationary deflagration front propagating inwards. The features of this front are discussed. A possibility of mass loss is indicated.

AB - We follow the accretion of hydrogen-rich matter onto the surface of a white dwarf in a close binary system. Two phases of accretion are assumed. First-slow accretion from the interstellar clouds, second-fast accretion from the companion. Hydrogen is ignited at the interface between the fast and slowly accreted layers. After a short runaway burning continues in the form of quasistationary deflagration front propagating inwards. The features of this front are discussed. A possibility of mass loss is indicated.

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Hydrogen burning on a white dwarf accreting hydrogen in a binary system

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