Close binary systems before and after mass transfer. II - Semi-detached systems

Details Close binary systems before and after mass transfer. II - Semi-detached systems Close binary systems before and after mass transfer. II - Semi-detached systems

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..411d&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 2, Oct. 1980, p. 411-432. Fonds de la Recherche Fondamentale Collective

Astronomy and Astrophysics

Astrophysics

12

Astrophysics, Binary Stars, Mass Transfer, Stellar Evolution, Astronomical Catalogs, Stellar Luminosity, Stellar Mass Accretion, Stellar Mass Ejection

Scientific paper

Recent data on semi-detached systems are compared with general results of close binary computations to determine the origin of Algol-type systems (classical case A and case B results are considered). Both the conservative and the non-conservative mode of mass exchange are investigated. It is found that the assumption of considerable mass loss from the system gives satisfying agreement with the observations. It is also concluded that the calculation of an extensive homogeneous network of case A computations is needed

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