Advertisement

Astrophysics

, Volume 28, Issue 1, pp 95–98 | Cite as

Solution of NLTE problem for Mg I in the atmosphere of an M giant with chromosophere. I. Menzel coefficients

  • Ya. V. Pavlenko
Article

Keywords

Atmosphere 
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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

Literature Cited

  1. 1.
    J. R. Auman and J. E. J. Woodrow, Astrophys. J.,157, 795 (1975).Google Scholar
  2. 2.
    Ya. V. Pavlenko, Effects of Deviation from Local Thermodynamic Equilibrium in the Atmospheres of M giants [in Russian], Valgus, Tallin (1984).Google Scholar
  3. 3.
    S. L. Wright, Commun. Univ. London Obs.,76, 1 (1975).Google Scholar
  4. 4.
    T. Kipper and J. Sitska, Tartu Astrofüüs. Obs. Teated,64, 15 (1981).Google Scholar
  5. 5.
    T. R. Ayras and J. L. Linsky, Astrophys. J.,205, 874 (1976).Google Scholar
  6. 6.
    W. L. Kelch, S. L. Linsky, and G. S. Basri, Astrophys. J.,220, 962 (1978).Google Scholar
  7. 7.
    G. A. Gurzadyan, Stellar Atmospheres [in Russian], Nauka, Moscow (1985).Google Scholar
  8. 8.
    O. Gingerich, R. W. Noyes, W. Kalkoffen, and Y. Cuny, Solar Phys.,2, 347 (1971).Google Scholar
  9. 9.
    M. L. Auer and I. N. Heasley, Astrophys. J.,205, 165 (1976).Google Scholar
  10. 10.
    A. A. Boyarchuk, L. S. Lyubimkov, and N. A. Sakhibullin, Astrofizika,22, 339 (1984).Google Scholar

Copyright information

© Plenum Publishing Corporation 1988

Authors and Affiliations

  • Ya. V. Pavlenko

There are no affiliations available

Personalised recommendations