Case A evolution of massive close binary systems

Details Case A evolution of massive close binary systems Case A evolution of massive close binary systems

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..367n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 2, Sept. 1984, p. 367-387. Sponsorship: Ministry of Education, Sc

Astronomy and Astrophysics

Astrophysics

12

A Stars, B Stars, Binary Stars, Stellar Evolution, Stellar Mass, Hertzsprung-Russell Diagram, Mass Transfer, Stellar Models, Supermassive Stars

Scientific paper

The case-A evolution of close binary systems with total mass of 20.4 solar mas is investigated by following the evolution of both components simultaneously. The evolution is followed up to the stage at which a system overflows the outer critical surface or evolves into the phase of mode-Br mass transfer. It is found that the evolution of the systems can be classified into six types. The ranges of initial parameters which lead systems to each type of evolution are shown on the initial-parameter plane. The evolutionary features of each evolution type are described in detail.

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