Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002arep...46..765t&link_type=abstract
Astronomy Reports, Vol. 46, Issue 9, pp. 765-778
Astronomy and Astrophysics
Astronomy
2
Scientific paper
We show that semi-detached close binary systems with massive (4 25M &sun;) black holes are formed in the evolution of massive stellar binaries in which the initial mass of the primary exceeds ˜25M &sun;. The mass exchange in such systems is maintained by the nuclear evolution of the donor and by its magnetic and induced stellar winds. The donor in such systems can be a main-sequence star, subgiant, non-degenerate helium star, or white dwarf. The evolution of corresponding systems with black-hole masses of 10M &sun; is investigated.
Fedorova Alexandra V.
Tutukov Aleksandr V.
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