Determining parameters of cool giant stars by modeling spectrophotometric and interferometric observations using the SAtlas program

@article{Neilson2008DeterminingPO,
  title={Determining parameters of cool giant stars by modeling spectrophotometric and interferometric observations using the SAtlas program},
  author={H. Neilson and J. B. Lester},
  journal={Astronomy and Astrophysics},
  year={2008},
  volume={490},
  pages={807-810}
}
Context. Optical interferometry is a powerful tool for observing the intensity structure and angular diameter of stars. When combined with spectroscopy and/or spectrophotometry, interferometry provides a powerful constraint for model stellar atmospheres. Aims. The purpose of this work is to test the robustness of the spherically symmetric version of the Atlas stellar atmosphere program, SAtlas, using interferometric and spectrophotometric observations. Methods. Cubes (three dimensional grids… Expand
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