Explaining the Discrepancy between ``Empirical'' and Predicted Ionization in the Winds of O-stars

Details Explaining the Discrepancy between ``Empirical'' and Predicted Ionization in the Winds of O-stars Explaining the Discrepancy between ``Empirical'' and Predicted Ionization in the Winds of O-stars

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..332..264m&link_type=abstract

The Fate of the Most Massive Stars, ASP Conference Series, Vol. 332, Proceedings of the conference held 23-28 May, 2004 in Grand

Astronomy and Astrophysics

Astronomy

Scientific paper

Resonance lines in the UV are diagnostics of stellar wind properties,
and therefore the associated ionized species are of special interest.

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