A model for the origin of the anomalous and very bright UV lines of Fe II in gaseous condensations of the star $\mathsf{\eta}$ Carinae
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20011062/pdf
Reference23 articles.
1. The Escape of Resonance-Line Radiation from Extremely Opaque Media
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4. HST/GHRS Observations of the Compact Slow Ejecta of ETA Carinae
5. ETA CARINAE AND ITS ENVIRONMENT
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3. On the 1.7 μm Fe ii and other natural lasers;Monthly Notices of the Royal Astronomical Society;2010-03
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