J/A+A/417/375ivo://CDS.VizieR/J/A+A/417/375doi:10.26093/cds/vizier.34170375CDSMilovanovic N.Dimitrijevic M.S.Popovic L.C.Simic Z.2004-06-05T21:11:25Z2004-06-05T21:09:58ZCDS support team

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

cds-question@unistra.fratomic-physicsStark broadening parameters, widths and shifts, for 84 spectral lines of doubly-ionized cadmium (Cd III) have been calculated using the modified semi-empirical approach (MSE). Calculated spectral lines belong to the transitions 4d^9^5s-4d^9^5p and 4d^9^5p-4d^9^5d. Widths and shifts of the spectral lines are given for temperature range of 5000K-60000K and an electron density of 10^23^m^-3^. The influence of collisions with charged particles on Cd III UV stellar lines along the HR diagram is discussed. Compared to the Doppler broadening, the influence of the Stark broadening mechanism is more important for deeper atmospheric layers and for larger values of logg. Stark broadening does not depend on turbulent velocity for the considered stellar model of a standard main sequence hot star of A0 spectral type. The influence of the Stark widths for standard models of DA and DB white dwarfs is also discussed.2004A&A...417..375Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/417/375CatalogResearchIsServedByTAP VizieR generic servicerelated-toVI/82 : Stark broadening of H lines (Stehle 1995)J/A+A/400/791 : Stark broadening of Be III lines (Dimitrijevic+, 2003)J/A+AS/105/243 : Stark broadening of BeI lines (Dimitrijevic+ 1994)J/A+AS/105/245 : Stark broadening Al XI and Si XII (Dimitrijevic+ 1994)J/A+AS/107/349 : Stark broadening Ne VIII and Na IX (Dimitrijevic+, 1994)J/A+AS/109/551 : Stark broadening. XII. OIV + OV (Dimitrijevic+, 1995)J/A+AS/113/579 : Stark broadening of NV (Shoening+, 1995)J/A+AS/115/351 : Stark broadening. XIII. C V and P V (Dimitrijevic+, 1996)J/A+AS/116/359 : Stark broadening of Xe II lines (Popovic+, 1996)J/A+AS/117/127 : Stark broadening of solar MgI lines (Dimitrijevic+, 1996)J/A+AS/119/369 : Stark broadening. XIV: Be III and B III (Dimitrijevic+, 1996)J/A+AS/119/529 : Stark broadening : Sr I (Dimitrijevic+, 1996)J/A+AS/122/163 : Stark broadening of Ba I + Ba II (Dimitrijevic+ 1997)J/A+AS/122/285 : VCS Stark broadening tables for hydrogen (Lemke, 1997)J/A+AS/122/533 : Stark broadening of P IV spectral lines (Dimitrijevic+ 1997)J/A+AS/127/295 : Stark broadening of Kr II lines (Popovic+ 1998)J/A+AS/127/543 : Stark broadening of S V lines (Dimitrijevic+ 1998)J/A+AS/128/203 : Stark broadening of Mn, Ga + Ge multiplets (Popovic+ 1998)J/A+AS/128/359 : Stark broadening of Ca IX and Ca X lines (Dimitrijevic+ 1998)J/A+AS/129/155 : Stark broadening Si XI + Si XIII lines (Dimitrijevic+ 1998)J/A+AS/130/539 : Stark broadening of Na X (Dimitrijevic+ 1998)J/A+AS/131/141 : Stark broadening of O VII and Mg XI (Dimitrijevic+ 1998)J/A+AS/131/143 : Stark broadening Sc X + XI, Ti XI + XII (Dimitrijevic+ 1998)J/A+AS/133/227 : Stark broadening of K VIII and K IX (Dimitrijevic+ 1998)J/A+AS/140/191 : Stark broadening of Ca I (Dimitrijevic+, 1999)J/A+AS/140/193 : Stark broadening of Zn I (Dimitrijevic+, 1999)J/A+A/400/791 : Stark broadening of Be III (Dimitrijevic+ 2003)J/A+A/423/397 : Stark broadening of Si V (Ben Nessib+, 2004)J/A+A/425/1147 : Stark broadening of Ga I (Dimitrijevic+, 2004)J/A+A/441/391 : Stark broadening of Cd I spectral lines (Simic+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/417/375https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/417/375http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/417/375https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/417/375https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/417/375http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/417/375GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/417/375/table1*Stark full widths and shifts for Cd III lines calculated within the modified semi-empirical approachrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelengthnmem.wl;phys.atmol.transitionfloatTransTransitionmeta.id;phys.atmol.transitionTTemperatureKphys.temperatureintFWHMFWHM for electron impacts (1)nmspect.line.broad.StarkdoubledShift for electron impacts (2)nmspect.line.broad.StarkdoubleJ/A+A/417/375/table2Stark widths in rad/s per electron for T=10000K and constants logA0 and A1 as described in paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelengthnmem.wlfloatTransTransitionmeta.id;phys.atmol.transitionlogwStark width per electron (1)log(rad.s**-1)spect.line.broad.StarkdoublelogA0Constant A0 (2)stat.fit.paramdoubleA1Constant A1 (2)stat.fit.paramdouble