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Thermonuclear Runaways on Accreting Hot White Dwarfs

Published online by Cambridge University Press:  12 April 2016

Dina Prialnik  and
Oded Regev
Dina Prialnik
Affiliation:
Racah Institute of Physics, Hebrew University Jerusalem, Israel
Oded Regev
Affiliation:
Department of Astronomy, Columbia University New York, NY 10027, U.S.A.

Abstract

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Preliminary results of 1–D fully hydrodynamic numerical calculations including accretion and mass loss on a 1M ⊙ hot white dwarf are presented. For the case of Ṁ = 10−8 M ⊙/yr and Teff = 125000°K we get flashes of duration of ∼ 30 – 40 yrs which reccur every ∼ 1500 years. During each flash ∼ 6x10−6 M ⊙ is lost (∼ 40% of the accreted envelope.

Information

Type
Session 2. The Physics of the Symbiotic Phenomenon
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 171 - 172
Copyright
Copyright © Kluwer 1988

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