Table 2
Wall shape and location before and after iterating on the temperature structure.
| Model | Before iteration | RT | After iteration | |||
| M pl | α | w | rexp [rpl] | rexp [AU] | rpl [AU] | w |
|
|
||||||
| 2 | 10-4 | 0.17 | 1.6 | 17 | 10.6 | 0.21 |
| 5 | 5 × 10-4 | 0.20 | 1.8 | 18 | 10.2 | 0.27 |
| 10 | 10-3 | 0.23 | 2.0 | 19 | 9.6 | 0.28 |
| 20 | 2 × 10-3 | 0.26 | 2.3 | 21 | 9.2 | 0.33 |
| 40 | 10-2 | 0.35 | 2.9 | 28 | 9.8 | 0.36 |
| 60 | 2 × 10-2 | 0.36 | 3.0 | 29 | 9.7 | 0.37 |
Notes.The wall shape w and its location rexp are defined in Eq. (1). The location of the planet rpl follows from comparing the fitted wall location in the radiative transfer code (rexp in column RT) with that of the hydrodynamical simulation. This subset of models is highlighted by triangles in the parameter study of Fig. 7.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.