Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-26T03:35:42.014Z Has data issue: false hasContentIssue false
  • English
  • Français

A Modelling of Line Transfer in Supergiant Envelopes

Published online by Cambridge University Press:  19 July 2016

Krzysztof Gesicki
Krzysztof Gesicki*
Affiliation:
N. Copernicus Astronomical Center, Laboratory for Astrophysics, ul. Chopina 12/18, 87-100 Torun, Poland

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 computer code that solves the transfer equation in moving atmosphere is prepared for analysis of variability in circumstellar spectral lines. This model gives a theoretical line shape, which consists of a symmetric photospheric line and superposed on it a P-Cyg type component originated in the envelope. Comparison between calculated and observed line profiles will be used to analyze 6 A/mm spectra of F-K supergiants.

Type
III. Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 135 - 137
Copyright
Copyright © Kluwer 1988 

References

Bernat, A.P., Astrophys. J., 213, 756, (1977)CrossRefGoogle Scholar
Hagen, W., Astrophys. J. Suppl., 38, 1, (1978)CrossRefGoogle Scholar
Kunasz, P.B., Hummer, D.G., Mon. Not. R. Astr. Soc., 166, 57, (1974)Google Scholar
Lambert, D.L., Hinkle, K.H., Hall, D.N.B., Astrophys. J., 246, 636, (1981)Google Scholar
Sanner, F., Astrophys. J. Suppl., 32, 115, (1976)CrossRefGoogle Scholar
Sargent, W.L.W., Astrophys. J., 134, 142, (1961)CrossRefGoogle Scholar
Smolinski, J., Climenhaga, J.L., Proc. IAU Symp. No.116, (1965)Google Scholar