Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-24T09:52:34.281Z Has data issue: false hasContentIssue false
  • English
  • Français

Mass Transfer Characterization in Close Binary Stars

Published online by Cambridge University Press:  07 August 2017

J. M. García  and
A. Giménez
J. M. García
Affiliation:
Departamento de Física, Universidad Politécnica de Madrid Ronda de Valencia, 3. 28012 Madrid, Spain
A. Giménez
Affiliation:
Laboratorio de Astrofísica Espacial y Física Fundamental (INTA). Apartado 50727. 28080 Madrid, Spain

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.

A method for estimating representative values of the parameters that characterize the loss of mass and angular momentum occurred during the evolution of a close binary star is considered. Absolute dimensions previous to mass-transfer stage have been obtained for a select group of 43 semidetached systems adopting a grid of values of mass loss, angular momentum loss and initial mass ratio. Our study reveals a highly non-conservative scenario for the evolution towards an Algol-type system.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 337 - 340
Copyright
Copyright © Kluwer 1992 

References

Claret, A. and Giménez, A. (1989), Astron. Astrophys. Suppl. 81, 1.Google Scholar
Eggleton, P.P. (1983), Astrophys. J. 268, 368.Google Scholar
García, J.M. and Giménez, A. (1991), “A New Catalogue of Semidetached Algol-type Binaries with Well-Determined Absolute Parameters”, Communication to this Symposium.CrossRefGoogle Scholar
Harmanec, P. (1988), Bull. Astron. Inst. Czech. 39, 329.Google Scholar
Popper, D.M. (1980), Ann. Rev. Astron. Astrophys. 18, 115.Google Scholar
Vanveberen, D., De Greve, J.P., Van Dessel, E.L., De Loore, C. (1979), Astron. Atrophys. 73, 19.Google Scholar