No CrossRef data available.
Article contents
Disturbed Binaries: The Early Phases
Published online by Cambridge University Press: 14 August 2015
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.
The disturbance of components and system parameters by mass transfer during and at the end of core hydrogen burning, as well as at the onset of core helium burning is reviewed. Emphasis is given to the influence of the evolution of the gainer and to the variation of the chemical composition of the surface.
- Type
- Joint Discussions
- Information
- Copyright
- Copyright © Kluwer 1989
References
Andersen, J., Clausen, J.V., Nordstrom, B., Reipurth, B.: Astron. Astrophys. 121, 271.Google Scholar
Andersen, J., Clausen, J.V., Gustafsson, B., Nordstrom, B., Vandenberg, D.A.: 1988, preprint “Absolute dimensions of eclipsing binaries: XIII. AI Phoenicis: A case study in stellar evolution”.Google Scholar
De Greve, J.P., Packet, W.: 1988, in ‘Algols’, Batten, A.H. (ed.), IAU Coll. 107.CrossRefGoogle Scholar
Habets, G.M.H.J., Zwaan, C.: 1988, preprint “Asynchromous rotation in close binary systems with circular orbits”.Google Scholar
Savonije, G.J., Papaloizou, J.C.B.: 1985, in ‘Interacting Binaries’, Eggleton, P.P. and Pringle, J.E. (eds.), D. Reidel Publ. Co., Dordrecht, Holland, p. 83.Google Scholar