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On the outburst of symbiotic stars

Published online by Cambridge University Press:  12 April 2016

H. Nussbaumer  and
M. Vogel
H. Nussbaumer
Affiliation:
Institute of AstronomETH Zentrum 8092 Zürich, (Switzerland)
M. Vogel
Affiliation:
Institute of AstronomETH Zentrum 8092 Zürich, (Switzerland)

Summary

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The most commonly advocated models for explaining the outburst of symbiotic systems are thermonuclear runaways, modulated mass accretion through a disc, or accretion disc instabilities. We show that the onset of a strong stellar wind on the cool component can also produce the observed increase in luminosity.

Type
Session 2. The Physics of the Symbiotic Phenomenon
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 169 - 170
Copyright
Copyright © Kluwer 1988

References

Koester, D., Schönberner, D.: 1986, Astron.Astrophys. 154, 125 Google Scholar
Nussbaumer, H., Schmutz, W.: 1983, Astron.Astrophys. 126, 59 Google Scholar
Nussbaumer, H., Vogel, M.: 1987, Astron.Astrophys. 182, 51 Google Scholar