In a recently published paper Matsumura et al. (2010) (hereafter M10), we have studied the evolution of three-planet systems in dissipating gas disks by using a hybrid N-body and one-dimensional gas disk evolution code. In this article, we highlight some results which are only briefly mentioned in M10.
|Title of host publication||Proceedings of the International Astronomical Union|
|Number of pages||2|
|Publication status||Published - Oct 2010|
- n-body simulations
- planetary system: protoplanetary disks
- planetary systems : formation