The FERRUM project: Branching ratios and atomic transition probabilities of Fe II transitions from the 3d6(a 3F)4p subconfiguration in the visible to VUV spectral region
(2001) In Astronomy & Astrophysics 377. p.361-367- Abstract
- We report measurements of the relative intensities of 81 emission linesof Fe II between 160 nm and 350 nm (62 168 cm<SUP>-1</SUP> to 28 564cm<SUP>-1</SUP>) from 4 levels by high resolution Fourier transformspectrometry, using a Penning discharge lamp as light source. Theserelative intensities have been used to determine the line branchingfractions, which have then been combined with accurate experimentalradiative lifetime measurements reported recently to give absolutetransition probabilities and oscillator strengths for 81 lines. Theaccuracy of these f-values is compared with other previous experimentalmeasurements, and with theoretical values. The new transitionprobabilities will allow accurate determinations of... (More)
- We report measurements of the relative intensities of 81 emission linesof Fe II between 160 nm and 350 nm (62 168 cm<SUP>-1</SUP> to 28 564cm<SUP>-1</SUP>) from 4 levels by high resolution Fourier transformspectrometry, using a Penning discharge lamp as light source. Theserelative intensities have been used to determine the line branchingfractions, which have then been combined with accurate experimentalradiative lifetime measurements reported recently to give absolutetransition probabilities and oscillator strengths for 81 lines. Theaccuracy of these f-values is compared with other previous experimentalmeasurements, and with theoretical values. The new transitionprobabilities will allow accurate determinations of Fe II abundances ina wide variety of astrophysical objects. Tables 2 and 3 are onlyavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/377/361 (Less)
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/130152
- author
- Pickering, J. C. ; Johansson, Sveneric LU and Smith, P. L.
- organization
- publishing date
- 2001
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- ATOMIC DATA, LINE: IDENTIFICATION, TECHNIQUES: SPECTROSCOPIC, STARS: ABUNDANCES
- in
- Astronomy & Astrophysics
- volume
- 377
- pages
- 361 - 367
- publisher
- EDP Sciences
- external identifiers
-
- scopus:0035494129
- ISSN
- 0004-6361
- DOI
- 10.1051/0004-6361:20010943
- language
- English
- LU publication?
- yes
- id
- 105161db-6fc5-4b69-bfa4-239b456af050 (old id 130152)
- date added to LUP
- 2016-04-01 16:20:04
- date last changed
- 2022-12-12 18:10:18
@article{105161db-6fc5-4b69-bfa4-239b456af050, abstract = {{We report measurements of the relative intensities of 81 emission linesof Fe II between 160 nm and 350 nm (62 168 cm<SUP>-1</SUP> to 28 564cm<SUP>-1</SUP>) from 4 levels by high resolution Fourier transformspectrometry, using a Penning discharge lamp as light source. Theserelative intensities have been used to determine the line branchingfractions, which have then been combined with accurate experimentalradiative lifetime measurements reported recently to give absolutetransition probabilities and oscillator strengths for 81 lines. Theaccuracy of these f-values is compared with other previous experimentalmeasurements, and with theoretical values. The new transitionprobabilities will allow accurate determinations of Fe II abundances ina wide variety of astrophysical objects. Tables 2 and 3 are onlyavailable in electronic form at the CDS via anonymous ftp tocdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/377/361}}, author = {{Pickering, J. C. and Johansson, Sveneric and Smith, P. L.}}, issn = {{0004-6361}}, keywords = {{ATOMIC DATA; LINE: IDENTIFICATION; TECHNIQUES: SPECTROSCOPIC; STARS: ABUNDANCES}}, language = {{eng}}, pages = {{361--367}}, publisher = {{EDP Sciences}}, series = {{Astronomy & Astrophysics}}, title = {{The FERRUM project: Branching ratios and atomic transition probabilities of Fe II transitions from the 3d<sup>6</sup>(a <sup>3</sup>F)4p subconfiguration in the visible to VUV spectral region}}, url = {{https://lup.lub.lu.se/search/files/4640986/624123.pdf}}, doi = {{10.1051/0004-6361:20010943}}, volume = {{377}}, year = {{2001}}, }