Preprint
Giant planet formation from disk instability; cooling and heating
Abstract
We present the results of high resolution SPH simulations of the evolution of
gravitationally unstable protoplanetary disks. We report on calculations in
Authors
Mayer L; Wadsley J; Quinn T; Stadel J
Publication date
November 3, 2003
DOI
10.48550/arxiv.astro-ph/0311048
Preprint server
arXiv