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Synthetic Spectra for WN Stars

Published online by Cambridge University Press:  14 August 2015

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
Copyright
Copyright © Reidel 1982 

References

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Wehrse, R., 1981, Mon. Nat. R. astr. Soc. 195, 553.Google Scholar