J/A+A/423/397ivo://CDS.VizieR/J/A+A/423/397doi:10.26093/cds/vizier.34230397CDSBen Nessib N.Dimitrijevic M.S.Sahal-Brechot S.2004-10-11T21:29:59Z2004-10-11T21:21:29ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsUsing a semiclassical perturbation approach, we have obtained Stark broadening parameters for 16 Si V multiplets using atomic data calculated ab initio with the SUPERSTRUCTURE code. In order to complete Stark broadening data for the most important charged perturbers in stellar atmospheres, Stark broadening parameters for proton-, He II-, and Si II-impact line widths and shifts are also presented. Results have been obtained for an electron density of 10^17^cm^-3^ as a function of temperature. Moreover, we have performed the same calculations with oscillator strengths calculated within the Coulomb approximation.2004A&A...423..397Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/423/397CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/105/243 : BeI lines (Dimitrijevic+ 1994)J/A+AS/105/245 : Al XI and Si XII (Dimitrijevic+ 1994)J/A+AS/107/349 : Ne VIII and Na IX (Dimitrijevic+ 1994)J/A+AS/109/551 : OIV and OV (Dimitrijevic+ 1995)J/A+AS/115/351 : C V and P V (Dimitrijevic+, 1996)J/A+AS/116/359 : Xe II lines (Popovic+, 1996)J/A+AS/117/127 : solar Mg I lines (Dimitrijevic+, 1996)J/A+AS/119/369 : Be III and B III (Dimitrijevic+, 1996)J/A+AS/119/529 : Sr I spectral lines (Dimitrijevic+, 1996)J/A+AS/120/373 : Sc II, Y II and Zr II Stark width (Popovic+ 1996)J/A+AS/122/163 : Ba I and Ba II lines (Dimitrijevic+, 1996)J/A+AS/122/533 : P IV spectral lines (Dimitrijevic+, 1997)J/A+AS/127/295 : Kr II lines (Popovic+ 1998)J/A+AS/127/543 : S V lines (Dimitrijevic+ 1998)J/A+AS/128/203 : Mn, Ga & Ge multiplets (Popovic+ 1998)J/A+AS/128/359 : Ca IX and Ca X lines (Dimitrijevic+ 1998)J/A+AS/129/155 : Si XI and Si XIII lines (Dimitrijevic+ 1998)J/A+AS/130/539 : Na X (Dimitrijevic+ 1998)J/A+AS/131/141 : O VII and Mg XI (Dimitrijevic+ 1998)J/A+AS/131/143 : Sc X, Sc XI, Ti XI and Ti XII (Dimitrijevic+ 1998)J/A+AS/133/227 : K VIII and K IX (Dimitrijevic+ 1998)J/A+AS/140/191 : Ca I (Dimitrijevic+ 1999)J/A+AS/140/193 : Zn I (Dimitrijevic+ 1999)J/A+A/400/791 : Be III (Dimitrijevic+ 2003)J/A+A/417/375 : Cd III (Milovanovic+, 2004)J/A+A/425/1147 : Ga I (Dimitrijevic+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/423/397https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/423/397http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/423/397https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/423/397https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/423/397http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/423/397GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/423/397/table1*Stark broadening parameters due to e-impacts for Si VrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNPerturber densitycm**-3phys.densitydoubleElElementphys.atmol.elementcharTrTransitionmeta.id;phys.atmol.transitioncharlambdaWavelength0.1nmem.wlfloatCParameter C (G1)0.1nm.cm**-3stat.fit.paramdoubleTTemperatureKphys.temperaturedoubleWeFWHM for electron impacts (G2) (4)0.1nmspect.line.broad.Starkdoubledeshift for electron impacts (G3) (4)0.1nmspect.line.broad.StarkdoubleWpFWHM for electron impacts (G2) (5)0.1nmspect.line.broad.Starkdoubledpshift for electron impacts (G3) (5)0.1nmspect.line.broad.StarkdoubleJ/A+A/423/397/table2Stark broadening parameters due to p-, He II-, and Si II-impacts for Si VrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNPerturber densitycm**-3phys.densitydoubleElElementphys.atmol.elementcharTrTransitionmeta.id;phys.atmol.transitioncharlambdaWavelength0.1nmem.wlfloatCParameter C (G1)0.1nm.cm**-3stat.fit.paramdoubleTTemperatureKphys.temperaturedoubleWpFWHM for proton impacts (G2)0.1nmspect.line.broad.Starkdoubledpshift for proton impacts (G3)0.1nmspect.line.broad.StarkdoubleWHe++FWHM for He II-impacts (G2)0.1nmspect.line.broad.StarkdoubledHe++shift for He II-impacts (G3)0.1nmspect.line.broad.StarkdoubleWSi++FWHM for Si II-impacts (G2)0.1nmspect.line.broad.StarkdoubledSi++shift for Si II-impacts (G3)0.1nmspect.line.broad.Starkdouble