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Synthetic Spectra for WN Stars
Published online by Cambridge University Press: 14 August 2015
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
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- Copyright
- Copyright © Reidel 1982
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