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An empirical study of Wolf-Rayet stellar wind ionization stratification
Published online by Cambridge University Press: 07 August 2017
Abstract
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We present an analysis of high resolution UV (IUE) and optical (INT, AAT and ESO) spectroscopy of eight galactic WN and WC stars. We examine the correlation between ionization potential (IP) and the velocity structure of the stellar winds and find important correlations between line-width, IP and excitation potential (EP). These results provide potential constraints on the velocity law used in models of WR atmospheres.
- Type
- Session II - Model atmospheres for single Wolf-Rayet stars
- Information
- Copyright
- Copyright © Kluwer 1995
References
Kuhi, L.V.
1973, in: Bappu, M.K.V. & Sahade, J. (eds), Wolf-Rayet Stars and High Temperature Stars,
Proc. IAU Symp. No. 49
, (Dordrecht: Reidel), p. 205
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