The evolution of multiple planets in radiative disks

Details The evolution of multiple planets in radiative disks The evolution of multiple planets in radiative disks

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1379k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1379

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Scientific paper

Among the observed extrasolar planetary systems there is a high fraction of resonant configurations, which are believed to have formed through a convergent migration process. Here, the differential drift of planets in disks leads to a reduction in radial distance and eventual resonant capture. The final resonance that is reached depends on the physical parameter of the disk and the embedded planets. We will present various outcomes of such a migration process for a pair of planets in isothermal and radiative disks, which will be directly compared to known extrasolar systems.

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