O II Stark broadening parameters

DOI

Using a modified semiempirical approach, we have calculated Stark broadening full widths at half maximum for 25 OII multiplets for temperatures from 5000K up to 80000K using the needed oscillator strengths from the sophisticated atomic structure data base TOPbase. Then we compared our results with experimental data for 41 OII spectral lines and with the available semi-classical calculations to test the applied method and the accuracy of the results obtained.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34340773
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/434/773
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/773
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/434/773
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/434/773
Provenance
Creator Mahmoudi W.F.; Ben Nessib N.; Dimitrijevic M.S.
Publisher CDS
Publication Year 2005
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics