Other
Scientific paper
May 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003dps....35.0705l&link_type=abstract
American Astronomical Society, DPS meeting #35, #07.05; Bulletin of the American Astronomical Society, Vol. 35, p.922
Other
Scientific paper
We present fully self-consistent 3D Smoothed-Particle Hydrodynamics simulations of an isothermal gaseous circumstellar disk interacting with an embedded protoplanet. We calculate planet migration and accretion rates as a function of initial disk and planet masses. The rates are higher than previous analytic and numerical work has found, and we explore the discrepancy resulting from self-gravity, the vertical dimension, and adaptive spatial resolution. Under certain initial conditions the embedded planet can trigger gravitational instabilities, leading to further planet formation that would not occur in the absence of the first planet. Visualizations of each scenario are presented.
Governato Fabio
Lufkin Graeme
Quinn Terry
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