Mass transfer in a low mass semidetached binary, taking into consideration nonequilibrium effects

Details Mass transfer in a low mass semidetached binary, taking into consideration nonequilibrium effects Mass transfer in a low mass semidetached binary, taking into consideration nonequilibrium effects

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...114..407h&link_type=abstract

Astronomy and Astrophysics, vol. 114, no. 2, Oct. 1982, p. 407, 408.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Mass Transfer, Stellar Mass Accretion, Stellar Mass Ejection, Mass Ratios, Nonequilibrium Conditions, Radii

Scientific paper

Using a stepwise constant approximation for the response function, mass transfer has been calculated for a semidetached binary with the initial masses m1 = 0.8 solar mass and m2 = 0.6 solar mass. Taking into consideration nonequilibrium effects on the secondary's radius as well, it is shown that 'case A' mass transfer in a low mass binary does not necessarily lead to a contact system.

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