Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.134..219n&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 134, no. 2, June 1987, p. 219-234.
Astronomy and Astrophysics
Astrophysics
4
Binary Stars, Mass Transfer, Stellar Evolution, Stellar Mass Accretion, Stellar Mass Ejection, Stellar Models
Scientific paper
The evolution of three close binary systems of total mass 20.4 M_sun; in and after the phase of mode Br mass-transfer in case A of mass exchange is investigated. In every case a secondary component evolves to interfere with the progress of primary's evolution and the system overflows the outer critical surface before the primary completes its nuclear-burning evolution. This strongly indicates the importance of simultaneous calculation of both components. A summary of evolution of the systems considered in this series of papers up to the stage of L2-overflow is given. The observational aspects of the numerical models are also discussed.
Nakamura Masaomi
Nakamura Yasuhisa
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