EDP Sciences
Free Access
Volume 397, Number 3, January III 2003
Page(s) 1143 - 1149
Section Celestial mechanics and astrometry
DOI https://doi.org/10.1051/0004-6361:20021557

A&A 397, 1143-1149 (2003)
DOI: 10.1051/0004-6361:20021557

The FERRUM Project: Experimental transition probabilities of [Fe II] and astrophysical applications

H. Hartman1, A. Derkatch2, M. P. Donnelly3, T. Gull4, A. Hibbert3, S. Johansson1, H. Lundberg5, S. Mannervik2, L.-O. Norlin6, D. Rostohar2, P. Royen2 and P. Schef2

1  Atomic Astrophysics, Lund Observatory, Lund University, Box 188, 221 00 Lund, Sweden
2  Physics Department, Stockholm University, AlbaNova University Center, 106 91 Stockholm, Sweden
3  Department of Applied Mathematics and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland
4  NASA/Goddard Space Flight Center, Code 681, Greenbelt, MD 20771, USA
5  Department of Physics, Lund Institute of Technology, Box 118, 221 00 Lund, Sweden
6  Physics Department, Royal Institute of Technology, AlbaNova University Center, 106 91 Stockholm, Sweden

(Received 10 September 2002 / Accepted 25 October 2002)

We report on experimental transition probabilities for thirteen forbidden [Fe II] lines originating from three different metastable $\ion{Fe}{ii}$ levels. Radiative lifetimes have been measured of two metastable states by applying a laser probing technique on a stored ion beam. Branching ratios for the radiative decay channels, i.e. M1 and E2 transitions, are derived from observed intensity ratios of forbidden lines in astrophysical spectra and compared with theoretical data. The lifetimes and branching ratios are combined to derive absolute transition probabilities, A-values.

We present the first experimental lifetime values for the two Fe II levels a4G 9/2 and b2H 11/2 and A-values for 13 forbidden transitions from a6S 5/2, a4G 9/2 and b4D 7/2 in the optical region. A discrepancy between the measured and calculated values of the lifetime for the b2H 11/2 level is discussed in terms of level mixing. We have used the code CIV3 to calculate transition probabilities of the a6D- a6S transitions.

We have also studied observational branching ratios for lines from 5 other metastable Fe II levels and compared them to calculated values. A consistency in the deviation between calibrated observational intensity ratios and theoretical branching ratios for lines in a wider wavelength region supports the use of [Fe II] lines for determination of reddening.

Key words: atomic data -- stars: individual: Eta Carinae -- ISM: dust, extinction

Offprint request: H. Hartman, Henrik.Hartman@astro.lu.se

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© ESO 2003

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