Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-17T19:11:30.459Z Has data issue: false hasContentIssue false
  • English
  • Français

The Evolution of Massive Close Binary Systems : Estimates of the Parameters Governing Mass and Angular Momentum Loss

Published online by Cambridge University Press:  14 August 2015

D. Vanbeveren  and
C. De Loore
D. Vanbeveren
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium
C. De Loore
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Brussels, Belgium

Extract

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.

It becomes more and more evident that for close binary evolution during Roche lobe overflow as well mass transfer as mass loss occurs. When a mass element ΔM is expelled from the primary during this phase, a fraction β is transferred to the secondary; the remaining part leaves the system. Moreover, angular momentum leaves the system, and also this fraction has to be specified; this fraction is related to a parameter α (Vanbeveren et al., 1979). For the computation of the evolution of massive close binaries also mass loss due to stellar wind of both components, prior to the Roche lobe overflow has to be taken into account. The mass loss rate Ṁ due to radiation driven stellar winds can be expressed as

Type
III. Mass Transfer and Mass Loss - Theory
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 115 - 121
Copyright
Copyright © Reidel 1980 

References

Batten, A.H.: 1967, Sixth Catalogue of the Orbital Elements of Spectroscopic Binary Systems, Publ.Dom.Astrophys.Obs., Vol. XIII, No.8.Google Scholar
Batten, A.H.: 1968, Astron.J. 73, 1.CrossRefGoogle Scholar
Bohannan, B., Conti, P.S.: 1976, Astrophys. J. 204, 797.CrossRefGoogle Scholar
Bracher, K., 1967, , .Google Scholar
Conti, P.S., Cowley, A.P., Johnson, G.B.: 1975, Publ. Astron. Soc. Pac. 87, 327.Google Scholar
Cowley, A.P., Hiltner, W.H., Berry, C.: 1971, Astron. Astrophys. 11., 407.Google Scholar
Crampton, D., Redman, R.O.: 1975, Astron. J. 80, 454.Google Scholar
de Loore, C., De Grève, J.P., Lamers, H.J.G.L.M.: 1977, Astron. Astrophys. 61, 251.Google Scholar
de Loore, C., De Grève, J.P., Vanbeveren, D.: 1978, Astron. Astrophys. 67, 373.Google Scholar
Evans, T.L.: 1979, Mon. Not. Roy. Astr. Soc. 186, 13.Google Scholar
Ganesh, K.S., Bappu, M.K.V., Natarijan, V.: 1967, Kodaikanal Obs.Bull. No. 184.Google Scholar
Garmany, K.: 1979, this symposium.Google Scholar
Hill, G., Crawford, D.L., Barnes, J.V.: 1974, Astron.J. 79, 1271.Google Scholar
Hutchings, J.B.: 1977, Publ. Astron. Soc. Pac. 89, 668.Google Scholar
Hutchings, J.B., Crampton, D., Cowley, A.P.: 1978, Astrophys. J. 225, 548.CrossRefGoogle Scholar
Lamers, H.J.G.L.M., Paerels, F., de Loore, C.: 1979, preprint.Google Scholar
Koch, R.H., Plavec, M., Wood, F.B.: 1970, Univ. of Pennsylvania, Pub. 10.Google Scholar
Massey, P., Conti, P.S.: 1977, Astrophys. J. 218, 431.Google Scholar
Massey, P., Conti, P.S.: 1979, in “Mass Loss and Evolution of O-Type Stars”, eds. Conti, P.S. and de Loore, C., Reidel, Dordrecht.Google Scholar
McCluskey, G.E., Kondo, Y.: 1972, Astrophys. Space Sci. 17, 134.Google Scholar
Niemela, V.S.: 1976, Astrophys. Space Sci. 45, 191.Google Scholar
Niemela, V.S., Sahade, J.: 1979, in “Mass Loss and Evolution of O-Type Stars”, eds. Conti, P.S. and de Loore, C., Reidel, Dordrecht.Google Scholar
Seggewiss, W.: 1974, Astron.Astrophys. 31., 211.Google Scholar
Stempien, K.: 1970, Acta Astron. 20, 117.Google Scholar
Stothers, R.: 1972, Astrophys. J. 175, 431.Google Scholar
Vanbeveren, D., De Grève, J.P., van Dessel, E.L., de Loore, C. 1979, Astron.Astrophys. 73, 19.Google Scholar
Vanbeveren, D., De Grève, J.P.: 1979, Astron.Astrophys (in press).Google Scholar
Vanbeveren, D., Packet, W.: 1979, Astron.Astrophys. (in press) Google Scholar
Woodward, E.J., Koch, R.H.: 1975, Astron.J. 87, 901.Google Scholar