Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T04:15:46.404Z Has data issue: false hasContentIssue false

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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