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Oscillator Strengths of Near-Infrared Lines of Fe II

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© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation G. Corrégé and A. Hibbert 2006 ApJ 636 1166 DOI 10.1086/497953

0004-637X/636/2/1166

Abstract

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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10.1086/497953