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Evolution of planetary systems in dissipating gas disks
Published online by Cambridge University Press: 10 November 2011
Abstract
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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.
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- Copyright © International Astronomical Union 2011
References
Chatterjee, S., Ford, E. B., Matsumura, S., & Rasio, F. A. 2008, ApJ, 686, 580CrossRefGoogle Scholar
Matsumura, S., Thommes, E. W., Chatterjee, S., & Rasio, F. A. 2010, ApJ, 714, 194CrossRefGoogle Scholar
Naoz, S., Farr, W. M., Lithwick, Y., Rasio, F. A., & Teyssandier, J. 2011, Nature, 473, 187CrossRefGoogle Scholar
Triaud, A. H. M. J., Cameron, A. C., Queloz, D., Anderson, D. R., et al. 2010, A&A, 524, A25Google Scholar
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