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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

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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.

Information

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

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