The origin of planetary system architectures – I. Multiple planet traps in gaseous discs

@article{Hasegawa2011TheOO,
  title={The origin of planetary system architectures – I. Multiple planet traps in gaseous discs},
  author={Yasuhiro Hasegawa and Ralph Egon Pudritz},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2011},
  volume={417},
  pages={1236-1259}
}
The structure of planetary systems around their host stars depends on their initial formation conditions. Massive planets will likely be formed as a consequence of rapid migration of planetesimals and low mass cores into specific trapping sites in protoplanetary discs. We present analytical modeling of inhomogeneities in protoplanetary discs around a variety of young stars, - from Herbig Ae/Be to classical T Tauri and down to M stars, - and show how they give rise to planet traps. The positions… Expand
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