On the eccentricity of self-gravitating circumstellar disks in eccentric binary systems
Earth and Planetary Astrophysics
2015-05-13 v2
Abstract
We study the evolution of circumstellar massive disks around the primary star of a binary system focusing on the computation of disk eccentricity. In particular, we concentrate on its dependence on the binary eccentricity. Self-gravity is included in our numerical simulations. Our standard model assumes a semimajor axis for the binary of 30 AU, the most probable value according to the present binary statistics.
Keywords
Cite
@article{arxiv.0908.0808,
title = {On the eccentricity of self-gravitating circumstellar disks in eccentric binary systems},
author = {F. Marzari and H. Scholl and P. Thebault and C. Baruteau},
journal= {arXiv preprint arXiv:0908.0808},
year = {2015}
}
Comments
Accepted for publication on A&A