Evolution of planetary systems in dissipating gas disks

Soko Matsumura, Edward W. Thommes, Sourav Chatterjee, Frederic A. Rasio

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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 languageEnglish (US)
Title of host publicationThe Astrophysics of Planetary Systems
Subtitle of host publicationFormation, Structure, and Dynamical Evolution
EditorsAlessandro Sozzetti, Mario Lattanzi, Alan Boss
Pages504-505
Number of pages2
EditionS276
DOIs
StatePublished - Oct 1 2010

Publication series

NameProceedings of the International Astronomical Union
NumberS276
Volume6
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

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Keywords

  • Methods: n-body simulations
  • Planetary systems: formation
  • Planetary systems: protoplanetary disks

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Cite this

Matsumura, S., Thommes, E. W., Chatterjee, S., & Rasio, F. A. (2010). Evolution of planetary systems in dissipating gas disks. In A. Sozzetti, M. Lattanzi, & A. Boss (Eds.), The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution (S276 ed., pp. 504-505). (Proceedings of the International Astronomical Union; Vol. 6, No. S276). https://doi.org/10.1017/S1743921311020989