Free Access
Table 2
Models used for the calculation of the absorption shown in Fig. 3.
| Model | Turbulent | LOS components | Lower | Gas radial |
|---|---|---|---|---|
| broadening(a) | boundary layer | velocity | ||
| HD 189733 b | ||||
| A | No | –3.5 km s−1 (100%) | Yes | This model(b) |
| B | Yes | –12 km s−1 (25%), –3.5 km s−1 (47%), 5 km s−1 (28%), | No | This model(b) |
| C | Yes | –12 km s−1 (25%), –3.5 km s−1 (47%), 5 km s−1 (28%), | Yes | This model(b) |
| D | No | –3.5 km s−1 (100%) | Yes | 40 km s−1(c) |
| GJ 3470 b | ||||
| E | Yes | No component | Yes | No velocities |
| F | Yes | –3.2 km s−1 ∀z | Yes | This model |
| G | Yes | No component at z < Rlobe, –5 km s−1 at z > Rlobe | Yes | This model |
Notes. (a) Doppler broadening was included in all models. (b)From the hydrodynamic model of this work. The gas radial velocities for this planet have negligible effects. (c) As in Seidel et al. (2020).
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.