Physics
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..797..537b&link_type=abstract
INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP Conference Proceedings, Volume 797, pp. 537-540 (2005).
Physics
Binary Stars, Radiation Effects, Stellar Structure, Stellar Evolution, Spectroscopic Binaries, Close Binaries, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages
Scientific paper
Irradiation of the secondaries in close binary systems affects their appearance and can drastically change their internal structure and hence long-term evolution. We have developed a three-dimensional fluid dynamics code for modelling these effects. We give particular emphasis to the role of circulation driven by the external heating and the radiative surface stress. We present results of self-consistent calculations for the circulation in irradiated systems and show how the inclusion of these is vital to the understanding and interpretation of any system where external irradiation of the secondary is significant.
Beer Martin E.
Podsiadlowski Philipp
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