New Fe ii energy levels from stellar spectra
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201015126/pdf
Reference13 articles.
1. Ultraviolet doubly excited Fe II lines in the laboratory and in the A-type star 21 Pegasi
2. The lowest 5g-6h supermultiplet of Fe II
3. New identified (3H)4d–(3H)4f transitions of Fe II from UVES spectra of HR 6000 and 46 Aquilae
4. A refined analysis of the remarkable Bp star HR 6000
5. Unidentified lines in the spectra of two iron overabundant CP stars: are they FeII lines?
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