Accretion onto ZAMS stars - Application to beta Lyrae and remarks on X-ray binaries

Details Accretion onto ZAMS stars - Application to beta Lyrae and remarks on X-ray binaries Accretion onto ZAMS stars - Application to beta Lyrae and remarks on X-ray binaries

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....75..255p&link_type=abstract

Astronomy and Astrophysics, vol. 75, no. 1-2, May 1979, p. 255-257. Research supported by the Fonds de la Recherche Fondamental

Astronomy and Astrophysics

Astrophysics

25

Eclipsing Binary Stars, Main Sequence Stars, Stellar Evolution, Stellar Mass Accretion, X Ray Binaries, X Ray Sources, Mass Transfer, Roche Limit, Stellar Mass

Scientific paper

Computations are performed for secondary components undergoing accretion during the mass exchange phase in close binary systems. As a result it is shown that the parameters of theoretical models for binary systems, such as beta Lyrae and X-ray binaries, imply that these systems pass through a contact phase, putting constraints on the predicted parameters of the ancestor systems.

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