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The FERRUM project: transition probabilities for forbidden lines in [Fe II] and experimental metastable lifetimes
Department of Physics, Stockholm University, AlbaNova University Center, 10691 Stockholm, Sweden.
Lund Observatory, Lund University, Box 43, 22100 Lund, Sweden.ORCID-id: 0000-0001-9853-2555
Lund Observatory, Lund University, Box 43, 22100 Lund, Sweden.
Lund Observatory, Lund University, Box 43, 22100 Lund, Sweden.ORCID-id: 0000-0003-0375-6076
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2009 (engelsk)Inngår i: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 508, nr 1, s. 525-529Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

Context. Accurate transition probabilities for forbidden lines are important diagnostic parameters for low-density astrophysical plasmas. In this paper we present experimental atomic data for forbidden [Fe II] transitions that are observed as strong features in astrophysical spectra. Aims. We measure lifetimes for the 3d6 (3G)4sa4 and 3d 6 (3D)4sb4 D1/2 metastable levels in Fe II and experimental transition probabilities for the forbidden transitions 3d7a4F7/2,9/2-3d6( 3G)4sa4.Methods. The lifetimes were measured at the ion storage ring facility CRYRING using a laser probing technique. Astrophysical branching fractions were obtained from spectra of Eta Carinae, obtained with the Space Telescope Imaging Spectrograph onboard the Hubble Space Telescope. The lifetimes and branching fractions were combined to yield absolute transition probabilities.Results. The lifetimes of the a4G11/2 and the b4D1/2 levels have been measured and have the following values, r = 0.75 ± 0.10 s respectively. Furthermore, we have determined the transition probabilities for two forbidden transitions of a 4F7/2,9/2-a4G11/2 at 4243.97 and 4346.85Å. Both the lifetimes and the transition probabilities are compared to calculated values in the literature. 

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2009. Vol. 508, nr 1, s. 525-529
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URN: urn:nbn:se:mau:diva-63265DOI: 10.1051/0004-6361/200913233ISI: 000272417700054Scopus ID: 2-s2.0-71849114162OAI: oai:DiVA.org:mau-63265DiVA, id: diva2:1807691
Tilgjengelig fra: 2023-10-27 Laget: 2023-10-27 Sist oppdatert: 2023-10-27bibliografisk kontrollert

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Hartman, H.Nilsson, H.

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