Speaker
Lionel SIESS
(Université Libre de Bruxelles)
Description
We will present recent SPH simulations of common envelope evolution including the formation of dust. Our calculations indicate that radiative acceleration on dust grains has a weak impact on the dynamics of the gas. However, dust formation can significantly alter the observational properties of the object.
Primary author
Lionel SIESS
(Université Libre de Bruxelles)
