AmFm and lithium gap stars: Stellar evolution models with mass loss

  title={AmFm and lithium gap stars: Stellar evolution models with mass loss},
  author={M. Vick and G. Michaud and J. Richer and O. Richard},
  journal={arXiv: Solar and Stellar Astrophysics},
A thorough study of the effects of mass loss on internal and surface abundances of A and F stars is carried out in order to constrain mass loss rates for these stars, as well as further elucidate some of the processes which compete with atomic diffusion. Self-consistent stellar evolution models of 1.3 to 2.5 M_sun stars including atomic diffusion and radiative accelerations for all species within the OPAL opacity database were computed with mass loss and compared to observations as well as… Expand
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