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Models of late-type stellar photospheres

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Summary

In this review we discuss recent work and progress in the modelling of photospheres of stars of spectral types F and later. Special emphasis is laid on advances as regards the consideration of atomic and molecular blanketing, non-LTE and convection and other dynamic processes. In a special chapter we discuss the possibilities of semi-empirical modelling of late-type photospheres. In the conclusions we find that much important work remains in this field, but that a considerable part of this work may in fact be carried out in a near future.

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  1. Bengt Gustafsson

    Present address: Astronomiska Observatoriet, Box 515, S-75120, Uppsala, Sweden

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  1. Department of Astronomy, University of Texas at Austin, TX, USA

    Bengt Gustafsson

  2. Niels Bohr Institute, Blegdamsvej 17, DK-2100, Copenhagen, Denmark

    Uffe Gråe Jørgensen

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Gustafsson, B., Jørgensen, U.G. Models of late-type stellar photospheres. The Astron Astrophys Rev 6, 19–65 (1994). https://doi.org/10.1007/BF01208251

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