Table 1
Comparison between the mass-loss rates obtained from our hydrodynamic modelling (Col. 6), from the energy-limited formula (Col. 7), and from the literature (Col. 8).
| ID | Λ | d0 | FXUV | M* | Ṁ | Ṁen | Ṁpubl |
|---|---|---|---|---|---|---|---|
| (AU) | (erg cm−2 s−1) | (M⊙) | (g s−1) | (g s−1) | (g s−1) | ||
| HD 209458 b | 90 | 0.047 | 1086 | 1.148 | 1.2 × 1010 | 8.0 × 109 | 3.3 × 1010a |
| 0.6−10 × 1010b | |||||||
| 1.9 × 1010c | |||||||
| GJ 436 b | 58 | 0.02887 | 1760 | 0.452 | 3.95 × 109 | 2.9 × 109 | 1 × 108−1 × 109d |
| 1 × 1010e | |||||||
| 2.2 × 1010f | |||||||
| 4.5 × 109c | |||||||
| Kepler-11 b | 18 | 0.091 | 278 | 0.95 | 1.1 × 109 | 7.5 × 108 | 1.15−2 × 108g |
| 1.17−1.3 × 107h | |||||||
| 1 × 109e | |||||||
| HD 189733 b | 179 | 0.03 | 24778 | 0.8 | 4.9 × 109 | 4.8 × 1010 | 0.04−10 × 1010b |
| 5−9 × 1011e | |||||||
| 4.1 × 109c | |||||||
Notes. The final column lists also the source of the published mass-loss rates. (a) Murray-Clay et al. (2009); (b) Bourrier & Lecavelier des Etangs (2013); (c)Salz et al. (2016); (d)Ehrenreich et al. (2015); (e)Guo & Ben-Jaffel (2016); (f)Bourrier et al. (2016); (g)Lammer et al. (2013); (h)Kislyakova et al. (2014).
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