Skip to main content
Log in

Theoretical profiles of balmer lines in the spectra of stars with moving envelopes with allowance for spectral dependence of the hydrogen absorption coefficient

  • Published:
Astrophysics Aims and scope

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Literature Cited

  1. M. A. Pogodin, Astrofizika,24, 491 (1986).

    Google Scholar 

  2. V. V. Sobolev, Moving Envelopes of Stars [in Russian], Leningrad State University, Leningrad (1947).

    Google Scholar 

  3. W. R. Hannan, Astron. Astrophys.93, 353 (1981).

    Google Scholar 

  4. N. N. Chugai, Pis'ma Astron. Zh.,6, 166 (1980).

    Google Scholar 

  5. C. Bertout, Astrophys. J.,285, 269 (1984).

    Google Scholar 

  6. H. J. G. L. M. Lamers, M. Cerruti Sola, and M. Perinotto, Astrophys. J.,314, 726 (1987).

    Google Scholar 

  7. U. Finkenzeller and R. Mundt, Astron. Astrophys. Suppl. Ser.,55, 109 (1984).

    Google Scholar 

  8. A. A. Boyarchuk, Vopr. Kosmog.,7, 231 (1960).

    Google Scholar 

Download references

Authors

Additional information

Principal Astronomical Observatory, USSR Academy of Sciences. Translated from Astrofizika, Vol. 31, No. 1, pp. 150–161, July–August, 1989.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Pogodin, M.A. Theoretical profiles of balmer lines in the spectra of stars with moving envelopes with allowance for spectral dependence of the hydrogen absorption coefficient. Astrophysics 31, 506–513 (1989). https://doi.org/10.1007/BF01004399

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01004399

Keywords

Navigation