Giant Planet Migration, Disk Evolution, and the Origin of Transitional Disks

We present models of giant planet migration in evolving protoplanetary disks. Our disks evolve subject to viscous transport of angular momentum and photoevaporation, while planets undergo Type II migration. We use a Monte Carlo approach, running large numbers of models with a range in initial condit...

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Veröffentlicht in:	The Astrophysical journal 2009-10, Vol.704 (2), p.989-1001
Hauptverfasser:	Alexander, Richard D, Armitage, Philip J
Format:	Artikel
Sprache:	eng
Schlagworte:	ACCRETION DISKS ANGULAR MOMENTUM Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CALCULATION METHODS DISTRIBUTION Earth, ocean, space Exact sciences and technology JUPITER PLANET MASS MONTE CARLO METHOD ORBITS PLANETS PROTOPLANETS SPATIAL DISTRIBUTION
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