Abstract
Classic modeling techniques cannot be used to analyze Wolf-Rayet (W-R) spectra. At a minimum one must consider spherical geometry, non-LTE, and the transfer of radiation in an expanding atmosphere. A code incorporating all of these is briefly described. New atomic...
Cite
CITATION STYLE
APA
Hillier, D. J. (1991). Diagnostics of Wolf-Rayet Atmospheres. In Stellar Atmospheres: Beyond Classical Models (pp. 317–329). Springer Netherlands. https://doi.org/10.1007/978-94-011-3554-2_30
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