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The warm wind model

Published online by Cambridge University Press:  14 August 2015

Henny J.G.L.M. Lamers
Henny J.G.L.M. Lamers*
Affiliation:
The Astronomical Institute at Utrecht Space Research Laboratory

Abstract

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The analysis of the UV spectra of τ Sco (BO V) and ζ Pup (O4 f) resulted in the empirical warm wind model. In this model the presence of O5+ and N4+ ions in the envelopes of early type stars is explained by collisional ionization in a ‘warm’ envelope of T ≃ 2 105 K.

Information

Type
Session 4: Panel Discussion on Stellar Wind Theories
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979, pp. 191 - 199
Copyright
Copyright © Reidel 1979 

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