Non-conservative evolution of massive binary systems.

Details Non-conservative evolution of massive binary systems. Non-conservative evolution of massive binary systems.

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pabei..17...58h&link_type=abstract

Prog. Astron., Vol. 17, No. 1, p. 58 - 65

Astronomy and Astrophysics

Astronomy

Binaries: Evolution, Binaries: Massive Stars, Stellar Evolution: Massive Stars, Stellar Winds: Massive Stars

Scientific paper

It is known that massive stars have a lot of special features, e.g., they have strong stellar winds and thus great mass loss, high surface temperature and strong radiation pressure, and will evolve into a supernova explosion. If a massive star is at the same time a component of a binary system, it will also be subjected to the effects of the gravitational and the radiation field of its companion star. Thus, the development of the theory of non-conservative evolution of massive binaries will encounter a series of very sophisticated problems.

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