Abstract
We have constructed a grid of 3D hydrodynamic simulations of deep convective and line-blanketed atmospheres. We have developed a new consistent method for computing and employing T(τ) relations from these simulations, as surface boundary conditions for 1D stellar structure models. These 1D models have, in turn, had their mixing-length, α, calibrated against the averaged structure of each of the simulations. Both α and T(τ) vary significantly with Teff and log g.
| Original language | English |
|---|---|
| Article number | 06064 |
| Journal | EPJ Web of Conferences |
| Volume | 101 |
| DOIs | |
| Publication status | Published - 23 Sept 2015 |
| Event | CoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution - Toulouse, France Duration: 6 Jul 2014 → 11 Jul 2014 |
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