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General Theory for Shell Flash and nova Explosion of Accreting White Dwarfs

Published online by Cambridge University Press:  12 April 2016

D. Sugimoto ,
M. Y. Fujimoto ,
K. Nariai  and
K. Nomoto
D. Sugimoto
Affiliation:
Department of Earth Science and Astronomy, College of General Education, University of Tokyo
M. Y. Fujimoto
Affiliation:
Takada Branch, Faculty of Education, Niigata university
K. Nariai
Affiliation:
Tokyo Astronomical Observatory, University of Tokyo
K. Nomoto
Affiliation:
Department of Physics, Ibaraki university

Extract

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It is now well known that an accreting white dwarf experiences a shell flash near its suface. Such phenomena are related with rekindling of white dwarfs, slow and fast nova explosions etc. depending on its strength. Though many authors computed evolution through such shell flashes, they treated them only under specific conditions.

Type
Colloquium Session IV
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 280 - 284
Copyright
Copyright © The University of Rochester 1979

References

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