Abstract
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.
Original language | English |
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Title of host publication | Proceedings of the International Astronomical Union |
Pages | 504-505 |
Number of pages | 2 |
Volume | 6 |
DOIs | |
Publication status | Published - Oct 2010 |
Keywords
- methods
- n-body simulations
- planetary system: protoplanetary disks
- planetary systems : formation