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2005ApJ...627L.157C - Astrophys. J., 627, L157-L159 (2005/July-2)
The oscillator strengths of Fe II λλ2507, 2509.
CORREGE G. and HIBBERT A.
Abstract (from CDS):
We present calculations of the oscillator strengths of Fe II λλ2507, 2509, which are the strongest observed lines in the emission spectrum of the B and D Weigelt blobs of η Carinae. Unlike previous determinations of these oscillator strengths, our results are compatible with the modeling undertaken by Verner et al.
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Journal keyword(s): Atomic Data
Simbad objects: 2
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