Preprint
Gravitational instability in binary protoplanetary disks; new constraints on giant planet formation
Abstract
We use high resolution 3D SPH simulations to study the evolution of
self-gravitating binary protoplanetary disks. Heating by shocks and cooling are
Authors
Mayer L; Wadsley J; Quinn T; Stadel J
Publication date
May 25, 2004
DOI
10.48550/arxiv.astro-ph/0405502
Preprint server
arXiv