In Situ and Ex Situ Formation Models of Kepler 11 Planets

@article{DAngelo2016InSA,
  title={In Situ and Ex Situ Formation Models of Kepler 11 Planets},
  author={G. D’Angelo and P. Bodenheimer},
  journal={The Astrophysical Journal},
  year={2016},
  volume={828},
  pages={33}
}
  • G. D’Angelo, P. Bodenheimer
  • Published 2016
  • Physics
  • The Astrophysical Journal
  • We present formation simulations of the six Kepler 11 planets. Models assume either in situ or ex situ assembly, the latter with migration, and are evolved to the estimated age of the system, 8 Gyr. Models combine detailed calculations of both the gaseous envelope and the condensed core structures, including accretion of gas and solids, of the disk's viscous and thermal evolution, including photo-evaporation and disk-planet interactions, and of the planets' evaporative mass loss after disk… CONTINUE READING
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