MASSET , F.

Context.Numerical simulations of planet-disk interactions are usually performed with hydro-codes that – because they consider only an annulus of the disk, over a 2D grid – cannot take into account the global evolution of the disk. However, the global evolution governs type II planetary migration, so that the accuracy of the planetary evolution...

Icarus, 181, pp. 587-604, http://dx.doi.org./10.1016/j.icarus.2005.10.007

Astrophysical Journal, 705, pp. L148-L152 (2009)

International audience

Astronomy and Astrophysics, 502, pp. 679-693 (2009)

Astronomy and Astrophysics, 478, pp. 929-937, http://dx.doi.org./10.1051/0004-6361:20078546

International audience

International audience