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Theoretical Emission-Line Profiles Computed at Ondřejov

Published online by Cambridge University Press:  14 August 2015

Svatopluk Kříž*
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia

Abstract

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A rotationally symmetrical disk-shaped envelope was considered and the steady-state equations for level populations solved using the escape probability approximation. The line profiles were then calculated and compared with observations.

Type
Part IV: Line Formation in Expanding Atmospheres
Copyright
Copyright © Reidel 1976 

References

Gray, F. G. and Marlborough, J. M.: 1974, Astrophys. J. Suppl. 27, 121.Google Scholar
Huang, S.-S.: 1973, Astrophys. J. 183, 541.Google Scholar
Johnson, L. C.: 1972, Astrophys. J. 174, 227.CrossRefGoogle Scholar
Kříž, S.: 1973, Bull. Astron. Inst. Czech. 25, 143.Google Scholar
Marlborough, J. M.: 1969, Astrophys. J. 156, 135.Google Scholar
Marlborough, J. M.: 1970, Astrophys. J. 159, 575.Google Scholar