The Surface of Stellar Models - Now with more 3D simulations!

Regner Trampedach, Jørgen Christensen-Dalsgaard, Martin Asplund, Robert F. Stein, Ake Nordlund

    Research output: Contribution to journalConference articlepeer-review

    2 Citations (Scopus)

    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 languageEnglish
    Article number06064
    JournalEPJ Web of Conferences
    Volume101
    DOIs
    Publication statusPublished - 23 Sept 2015
    EventCoRoT Symposium 3, Kepler KASC-7 Joint Meeting on Space Photometry Revolution - Toulouse, France
    Duration: 6 Jul 201411 Jul 2014

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