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On the eccentricity of self-gravitating circumstellar disks in eccentric binary systems

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.

preprint2009arXivOpen access
F. MarzariH. SchollP. ThebaultC. Baruteau
astro-ph.EP
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
Citations: 0Reviews: 0Saves: 0Code: not linkedDataset: not linkedInstitutions: 0

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F. MarzariH. SchollP. ThebaultC. Baruteau

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