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Theory of Stellar Atmospheres (Theorie des Atmospheres Stellaires)

  • L. Cram
  • R. Pallavacini
  • D. Dravins
  • I. Hubeny
  • W. Kalkofen
  • R. Kurucz
  • J. L. Linsky
  • S. Owocki
  • D. Sasselov
  • C. Schrijver
  • E. Simmoneau
  • R. Wehrse
  • K. Werner
  • L. A. Willson
Chapter
Part of the International Council of Scientific Unions / International Astronomical Union / Union Astronomique Internationale book series (IAUT, volume 23A)

Abstract

Consistently with a trend observed in recent past triennial reports, progress in the theory of stellar atmospheres continues to be made in two different directions: (i) the traditional areas of continuum and line radiation transfer, line blanketing, atomic physics and atmospheric structures controlled by the joint conditions of radiative and hydrostatic equilibrium, and (ii) in areas of emerging interest such as oscillations, winds and mass loss, chromospheres, coronae and magnetic phenomena.

Keywords

White Dwarf Model Atmosphere Stellar Atmosphere Asymptotic Giant Branch Star Stellar Corona 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1997

Authors and Affiliations

  • L. Cram
  • R. Pallavacini
  • D. Dravins
  • I. Hubeny
  • W. Kalkofen
  • R. Kurucz
  • J. L. Linsky
  • S. Owocki
  • D. Sasselov
  • C. Schrijver
  • E. Simmoneau
  • R. Wehrse
  • K. Werner
  • L. A. Willson

There are no affiliations available

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