Modelling Circumbinary Planets: The case of Kepler-38

The Paper

•   accepted version

Animations

•   The central Part of the disk
  - Locally isothermal Model disk model without a planet, the standard model in the paper, see Fig.4
  


•   Moving planet around binary Isothermal model
  - Locally isothermal Model disk model with an embedded planet, corresponding to the final phase where the planet is in the 5:1 resonance with the binary, see Figs.7 and 8.
  


•   Moving planet around binary Radiative model
  - Radiative disk model with an embedded planet, corresponding to the final phase, of the blue/green curve in Fig.17