Oscillator Strengths of Near-Infrared Lines of Fe II

Details Oscillator Strengths of Near-Infrared Lines of Fe II Oscillator Strengths of Near-Infrared Lines of Fe II

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006apj...636.1166c&link_type=abstract

The Astrophysical Journal, Volume 636, Issue 2, pp. 1166-1171.

Astronomy and Astrophysics

Astronomy

5

Atomic Data

Scientific paper

We present extensive configuration interaction calculations of oscillator strengths and transition rates of certain near-infrared emission lines of Fe II observed in the BD Weigelt blobs of η Carinae. Comparison is made between our work and results available in existing databases. We offer arguments in favor of our results being the most accurate, where differences occur.

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