Evolution of Migrating Planets Undergoing Gas Accretion

@article{DAngelo2008EvolutionOM,
  title={Evolution of Migrating Planets Undergoing Gas Accretion},
  author={Gennaro D’Angelo and Stephen H. Lubow},
  journal={The Astrophysical Journal},
  year={2008},
  volume={685},
  pages={560 - 583}
}
We analyze the orbital and mass evolution of planets that undergo runaway gas accretion by means of two- and three-dimensional hydrodynamic simulations. The disk torque distribution per unit disk mass as a function of radius provides an important diagnostic for the nature of the disk-planet interactions. We present results of simulations for mass-gaining, migrating planets. For planets with an initial mass of 5 M⊕, which are embedded in disks with standard parameters and which undergo runaway… 
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