Table 1
Exponential damping rate τinc (in orbits), obtained from our isothermal and fully radiative simulations for three studied cases of planets in discs compared with the linear rate, as given by Tanaka & Ward (2004).
| Linear 3D | Fixed orbit | Moving orbit | |
|
|
|||
| iso H/r = 0.037 | 14.2 | 27 | 23 |
| iso H/r = 0.05 | 47.25 | − | 53 |
| fully radiative | 27.7 | 20 | 26.5 |
Notes. Shown are results for planets on fixed orbits and for moving planets.
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