Numerical simulations of the GG Tau Circumbinary disk

Details Numerical simulations of the GG Tau Circumbinary disk Numerical simulations of the GG Tau Circumbinary disk

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..733p&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present the first 2D hydrodynamical simulations of the GG Tau circumbinary disk including self-gravity. These simulations match on many points the physical properties deduced from observations. We show that self-gravity is probably very important for the dynamical evolution of the system. In particular, we find that self-gravity noticeably affects the structure of the disk, the accretion rate onto the central binary and the orbital evolution of the binary.

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