No CrossRef data available.
Article contents
Wind Accretion and Interaction in Long Period Binary Systems
Published online by Cambridge University Press: 30 March 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Recent observations of the class of objects called symbiotic nova are reviewed. They are suggested to be widely-separated long-period binary systems undergoing mass exchange by wind accretion. Their radio, infrared, optical and X-ray properties are explained by a model of interacting winds.
- Type
- Joint Discussions
- Information
- Copyright
- Copyright © Reidel 1986
References
Allen, D.A.
1979, I.A.U. Colloquium 46, Changing Trends in Variable Star Research, ed. Bateson, F., Smak, J., and Urch, I. (Hamilton, New Zealand: University of Waikato), p. 167.Google Scholar
Puetter, R.C., Russell, R.W., Soifer, B.T., and Willner, S.P.
1978, Astrophys. J. (Letters), 223, L93.Google Scholar
Wallerstein, G., Willson, L.A., Salzer, J. and Brugel, E.
1984, Astron. Astrophys., 133, 137.Google Scholar
Willson, L.A., Wallerstein, G., Brugel, E.W., and Stencel, R.E.
1984, Astron. Astrophys., 133, 154.Google Scholar
You have
Access