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Synthetic Spectra for WN Stars

Published online by Cambridge University Press:  14 August 2015

R. Wehrse
R. Wehrse*
Affiliation:
Institut für Theoretische Astrophysik Im Neuenheimer Feld 294 D 6900 Heidelberg Germany

Abstract

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A computer program is described which calculates the structure and the radiation field (including high resolution spectra) of spherically extended and moving atmospheres. Some preliminary results for models of WN stars (L/L0= 105, M/M0= 10, Teff= 30 000 K, and M=3 · 10−5 MOy−1) are presented and discussed.

Type
SESSION 2 — THE CHEMISTRY OF THE WOLF-RAYET STARS
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 135 - 138
Copyright
Copyright © Reidel 1982 

References

Kurucz, R.L., 1979, Astrophys. J. Suppl. Ser. 40, 1.Google Scholar
Peraiah, A., Grant, I.P., 1973, J. Inst. Math. Applic. 12, 75.CrossRefGoogle Scholar
Wehrse, R., 1981, Mon. Nat. R. astr. Soc. 195, 553.Google Scholar