Issue |
EAS Publications Series
Volume 71-72, 2015
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
|
|
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Page(s) | 173 - 174 | |
Section | Binaries | |
DOI | https://doi.org/10.1051/eas/1571038 | |
Published online | 01 December 2015 |
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 173-174
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 173-174
3D Simulation of a Dust-Driven Wind In a Binary System
1 Institut d'Astronomie et d'Astrophysique (IAA), Université Libre de Bruxelles (ULB), CP 226, Boulevard du Triomphe, 1050 Brussels, Belgium
2 Institut für Theoretische Astrophysik, Zentrum für Astronomie, Universität Heidelberg, Albert-Ueberle-Straße 2, 69120 Heidelberg, Germany
3 Monash Center for Astrophysics, Monash University, Clayton, Vic 3800, Australia
We implemented 3D SPH models of stellar winds including a self-consistent treatment of dust formation, radiative cooling, and radiation pressure on dust grains.
© EAS, EDP Sciences, 2015