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2011

The Response of Giant Stars To Dynamical-Timescale Mass Loss

Passy, Jean-Claude, Herwig, Falk, Paxton, Bill

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We study the response of giant stars to mass loss.

One-dimensional simulations of red and asymptotic giant branch stars with mass loss rates from $10^{-3}$ up to a few \msun/yr show in no case any significant radius increase.
The largest radius increase of 0.2% was found in the case with the lowest mass loss rate.
For dynamical-timescale mass loss rates, that may be encountered during a common envelope phase, the evolution is not adiabatic.

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