AGB Evolution in Binary Systems

Details AGB Evolution in Binary Systems AGB Evolution in Binary Systems

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..265..173f&link_type=abstract

Post-AGB Objects as a Phase of Stellar Evolution, Proceedings of the Toruń Workshop held July 5-7, 2000. Edited by R. Szczerba a

Astronomy and Astrophysics

Astrophysics

Scientific paper

Results from numerical modelling of the AGB phase in binaries are presented. The method is to use single star evolutionary tracks and modify them by introducing binary interactions. Considered effects include enhancement of mass loss from the AGB primary, accretion of matter from the AGB wind onto the secondary, angular momentum loss from the system and angular momentum transfer between the binary components. Two different mass loss enhancement prescriptions are tested. An attempt to include magnetic effects is also made. The influence of various model parameters on the system evolution is briefly discussed.

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