Abstract
This paper reviews the basic physics of thermonuclear runaways on the surfaces of accreting white dwarf stars, with a special emphasis on understanding the evolution of symbiotic novae.
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© 1988 Kluwer Academic Publishers
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Kenyon, S.J. (1988). Thermonuclear Runaway Models for Symbiotic Novae. In: Mikolajewska, J., Friedjung, M., Kenyon, S.J., Viotti, R. (eds) The Symbiotic Phenomenon. Astrophysics and Space Science Library, vol 145. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2969-2_26
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DOI: https://doi.org/10.1007/978-94-009-2969-2_26
Publisher Name: Springer, Dordrecht
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