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2010A&A...524A..54D - Astronomy and Astrophysics, volume 524, A54-54 (2010/12-1)

Importance of level mixing on accurate [Fe II] transition rates.

DEB N.C. and HIBBERT A.

Abstract (from CDS):

In a very recent measurement Gurell et al. (2009A&A...508..525G) commented that while the theoretical lifetime of a4G5.5 is approximately one tenth of the lifetime of b2H5.5 the corresponding measurement shows this to be close to one fifth. This large discrepancy is attributed to the effect of inadequate level mixing in the theoretical calculations. The aim of this work is to make a detailed analysis of these level mixing effects on transitions from various lower levels to the a4G5.5 and b2H5.5 levels given in three previous calculations and in the present more extensive CI calculation. The CIV3 structure codes of Hibbert (1975, Comput. Phys. Commun., 9, 141) and Hibbert et al. (1991, Comput. Phys. Commun., 64, 455) are used in the present work, combined with our ``fine-tuning'' extrapolation process. The calculated mixing between the upper levels, obtained in previous calculations, is shown to be too weak. The stronger mixing determined in our work gives rise to a calculated lifetime for b2H5.5 within 3% of the measured value. On the other hand our calculated lifetime for a4G5.5 is around 20% lower than the measured value, which has fairly wide error bars. Our enhanced calculations explain the difference between previous calculations of the b2H5.5 lifetime and the recent measured value and confirm the latter. We also suggest a somewhat higher value than experiment for the lifetime of a4G5.5.

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Journal keyword(s): atomic data - atomic processes - methods: numerical - stars: individual: Eta Carinae

Simbad objects: 1

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