The FERRUM Project: New f-value Data for Fe II and Astrophysical ApplicationsDepartment of Applied Mathematics and Theoretical Physics, The Queens University of Belfast, Belfast, Northern Ireland.
Atomic Astrophysics, Lund Observatory, Box 43, SE-221 00 Lund, Sweden.
Institute for Atomic and Molecular Physics, University of Hannover, Hannover, Germany.
Department of Physics, Lund Institute of Technology, Lund, Sweden.
NASA / Goddard Space Flight Center, Greenbelt, Maryland, USA.
Atomic Astrophysics, Lund Observatory, Box 43, SE-221 00 Lund, Sweden.
Department of Physics, Lund Institute of Technology, Lund, Sweden.
Physics Department, Stockholm University, Stockholm, Sweden.
Physics Department, Royal Institute of Technology, Stockholm, Sweden.
Physics Department, Blackett Laboratory, Imperial College, London, UK.
Astronomical Institute "Anton Pannekoek", University of Amsterdam, Amsterdam, The Netherlands.
Physics Department, Stockholm University, Stockholm, Sweden.
Physics Department, Stockholm University, Stockholm, Sweden.
Fachbereich Physik, University of Kaislerslautern, Kaiserslautern, Germany.
Institute for Atomic and Molecular Physics, University of Hannover, Hannover, Germany.
Atomic Astrophysics, Lund Observatory, Box 43, SE-221 00 Lund, Sweden.
Harvard-Smithsonian Center for Astrophysics, Cambridge MA, USA.
Department of Physics, Lund Institute of Technology, Lund, Sweden.
Atomic Astrophysics, Lund Observatory, Box 43, SE-221 00 Lund, Sweden.
Show others and affiliations
2002 (English)In: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. T100, no 1, p. 71-71Article in journal (Refereed) Published
Abstract [en]
We present the FERRUM Project, an international collaboration aiming at a production and evaluation of oscillator strengths (transition probabilities) of selected spectral lines of singly ionized iron group elements, that are of astrophysical relevance. The results obtained include measurements and calculations of permitted and forbidden lines of Fe II. The data have been applied to both emission and absorption lines in astrophysical spectra. We make comparisons between experimental, theoretical and astrophysical f-values. We give a general review of the various measurements, and discuss the UV8 multiplet of Fe II around 1610 Å in detail.
Place, publisher, year, edition, pages
Institute of Physics Publishing (IOPP), 2002. Vol. T100, no 1, p. 71-71
National Category
Atom and Molecular Physics and Optics
Identifiers
URN: urn:nbn:se:mau:diva-63248DOI: 10.1238/physica.topical.100a00071ISI: 000177162500009OAI: oai:DiVA.org:mau-63248DiVA, id: diva2:1807663
2023-10-272023-10-272023-10-27Bibliographically approved