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Mass transfer in asymptotic-giant-branch binary systems

Published online by Cambridge University Press:  08 August 2017

Zhuo Chen Open the ORCID record for Zhuo Chen [Opens in a new window] ,
Adam Frank ,
Eric G. Blackman ,
Jason Nordhaus  and
Jonathan Carroll-Nellenback
Zhuo Chen
Affiliation:
Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627 email: zchen25@ur.rochester.edu
Adam Frank
Affiliation:
Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627 email: zchen25@ur.rochester.edu
Eric G. Blackman
Affiliation:
Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627 email: zchen25@ur.rochester.edu
Jason Nordhaus
Affiliation:
National Technical Institute for the Deaf, Rochester Institute of Technology, Rochester, NY 14623
Jonathan Carroll-Nellenback
Affiliation:
Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627 email: zchen25@ur.rochester.edu
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Abstract

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Binary stars can interact via mass transfer when one member (the primary) ascends onto a giant branch. The amount of gas ejected by the binary and the amount of gas accreted by the secondary over the lifetime of the primary influence the subsequent binary phenomenology. Some of the gas ejected by the binary will remain gravitationally bound and its distribution will be closely related to the formation of planetary nebulae. We investigate the nature of mass transfer in binary systems containing an AGB star by adding radiative transfer to the AstroBEAR AMR Hydro/MHD code.

Keywords

binaries: closemethod: numericalplanetary nebulae: generalstars: AGB and post-AGB
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 367 - 368
Copyright
Copyright © International Astronomical Union 2017 

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