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Accretion on CO White Dwarfs. Influence of the External Burning Shells on the Evolution

Published online by Cambridge University Press:  12 April 2016

M. Hernanz ,
J. José  and
J. Isern
M. Hernanz
Affiliation:
Departament de Física i Enginyeria Nuclear, ETSEIB (UPC), Diagonal 647, 08028 Barcelona, SPAIN Grup d’Astrofísica, Societat Catalana de Física, Institut d’Estudis Catalans.
J. José
Affiliation:
Departament de Física i Enginyeria Nuclear, FIB (UPC), Pau Gargallo 5, 08028 Barcelona, SPAIN Grup d’Astrofísica, Societat Catalana de Física, Institut d’Estudis Catalans.
J. Isern
Affiliation:
Centre d’Estudis Avançats (CSIC), Camí de Santa Bàrbara, 17300 Blanes, Girona, SPAIN Grup d’Astrofísica, Societat Catalana de Física, Institut d’Estudis Catalans.

Abstract

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The influence of accretion in the evolution of CO white dwarfs is calculated, up to the thermonuclear runaway, with a previous analysis of the H-He burning shell. For this later study, a two-zone model is developed, consisting of two thin shells in plane-parallel approximation. The influence in the inner core evolution is discussed.

Type
3. Theory
Information
International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 388 - 389
Copyright
Copyright © Springer-Verlag 1990

References

Hernanz, M., et al, 1988, Ap. J. 324, 331.Google Scholar
Nomoto, K., et al, 1985, Astron. & Ap. 149, 239.Google Scholar
Paczynski, B., 1983, Ap. J. 264, 282.Google Scholar