Table 1.
RHD simulations parameters.
| Simulation | M⋆ | log(L⋆/L⊙) | R⋆ | Teff | log g | tavg | σP | ⟨Px⟩ | ⟨Py⟩ |
|---|---|---|---|---|---|---|---|---|---|
| M⊙ | AU | K | (cgs) | yr | AU | AU | AU | ||
| st35gm04b1n001 | 5 | 4.61 | 2.77 | 3373 | −0.410 | 24.95 | 0.114 | −0.105 | 0.007 |
| st35gm04n38 (a) | 5 | 4.62 | 2.72 | 3414 | −0.400 | 11.45 | 0.113 | −0.010 | 0.136 |
| st35gm03n13 (b) | 12 | 4.95 | 3.95 | 3430 | −0.354 | 9.24 | 0.036 | 0.022 | 0.008 |
| st36gm00n06 (b) | 6 | 4.38 | 1.82 | 3660 | 0.009 | 7.23 | 0.022 | 0.021 | 0.026 |
| st36gm00n04 (b) | 5 | 4.39 | 1.80 | 3663 | 0.023 | 22.92 | 0.030 | 0.006 | 0.003 |
| st36gm00n05 (b) | 6 | 4.39 | 1.75 | 3710 | 0.047 | 3.75 | 0.031 | 0.011 | −0.006 |
Notes. The table shows the simulation name, the stellar mass M⋆, the average emitted luminosity L⋆, the average approximate stellar radius R⋆, effective temperature Teff, and surface gravity log g, and the time tavg used for the averaging. The last three columns are the standard deviation (σP) of the time-averaged values of the photo-center displacement and its coordinates ⟨Px⟩ and ⟨Py⟩.
Simulation presented in Chiavassa et al. (2022) and Kravchenko et al. (2019).
Simulation presented in Chiavassa et al. (2011a).
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.