The FERRUM Project: New f-value Data for Fe II and Astrophysical Applications
(2002) 7th International Colloquium on Atomic Spectra and Oscillator Strengths (ASOS 7) T100. p.71-80- Abstract
- 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 Šin detail.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/118071
- author
- organization
- publishing date
- 2002
- type
- Chapter in Book/Report/Conference proceeding
- publication status
- published
- subject
- keywords
- 32.70.Cs., 95.30Ky
- host publication
- Physica Scripta
- volume
- T100
- pages
- 71 - 80
- publisher
- The Royal Swedish Academy of Sciences
- conference name
- 7th International Colloquium on Atomic Spectra and Oscillator Strengths (ASOS 7)
- conference location
- Belfast, United Kingdom
- conference dates
- 2001-08-05 - 2001-08-09
- external identifiers
-
- scopus:0036078930
- ISSN
- 0281-1847
- DOI
- 10.1238/Physica.Topical.100a00071
- language
- English
- LU publication?
- yes
- id
- e9b8e5ad-46da-493f-90e2-0ccd80a1625b (old id 118071)
- date added to LUP
- 2016-04-01 15:36:56
- date last changed
- 2024-04-11 09:27:26
@inproceedings{e9b8e5ad-46da-493f-90e2-0ccd80a1625b, abstract = {{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 Šin detail.}}, author = {{Johansson, Sveneric and Derkatch, A. and Donnelly, M. P. and Hartman, Henrik and Hibbert, A. and Sabel, Hans and Kock, M. and Li, Zhongshan and Leckrone, D. S. and Litzén, Ulf and Lundberg, Hans and Mannervik, S. and Norlin, L-O. and Nilsson, Hampus and Pickering, J. and Taassen, T. and Rostohar, D. and Royen, P. and Schmitt, A. and Johanning, M. and Sikström, Carl Martin and Smith, P. L. and Svanberg, Sune and Wahlgren, Glenn}}, booktitle = {{Physica Scripta}}, issn = {{0281-1847}}, keywords = {{32.70.Cs.; 95.30Ky}}, language = {{eng}}, pages = {{71--80}}, publisher = {{The Royal Swedish Academy of Sciences}}, title = {{The FERRUM Project: New f-value Data for Fe II and Astrophysical Applications}}, url = {{https://lup.lub.lu.se/search/files/4432921/2370311.pdf}}, doi = {{10.1238/Physica.Topical.100a00071}}, volume = {{T100}}, year = {{2002}}, }