New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit

We present new models for low-mass stars down to the hydrogen-burning limit that consistently couple atmosphere and interior structures, thereby superseding the widely used BCAH98 models. The new models include updated molecular linelists and solar abundances, as well as atmospheric convection parameters calibrated on 2D/3D radiative hydrodynamics simulations. Comparison of these models with observations in various colour-magnitude diagrams for various ages shows significant improvement over previous generations of models. The new models can solve flaws that are present in the previous ones, such as the prediction of optical colours that are too blue compared to M dwarf observations. They can also reproduce…

• RS
  Royal Society
• AN
  Agence Nationale de la Recherche

  Award: ANR10-BLANC0504-01
• CN
  Centre National de la Recherche Scientifique
• SA
  Science and Technology Facilities Council

  Awards: FP7/2007-2013, ST/J001627/1