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Some Applications of Model Atmospheres

Published online by Cambridge University Press:  25 April 2016

M. S. Bessell
M. S. Bessell*
Affiliation:
Mount Stromlo and Siding Spring Observatory, Research School of Physical Sciences, Australian National University
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Extract

In the five years since the last invited paper on model stellar atmosphere applications there have been many significant advances made on all fronts. The five aspects which I will cover in this paper are:

  • (1) the results of white dwarf model atmosphere investigations;

  • (2) the results of the inclusion of non LTE phenomena in the atmosphere computations of hot (T > 15,000 K) stars;

  • (3) the probable understanding of the cause of peculiar abundance patterns in the Ap and Bp and Am stars;

  • (4) the advances in theory and observations of cool star atmospheres; and

  • (5) the use of synthetic spectra and colours.

Type
Invited Papers
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 5 , September 1974 , pp. 230 - 235
Copyright
Copyright © Astronomical Society of Australia 1974

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