J/A+A/399/795ivo://CDS.VizieR/J/A+A/399/795doi:10.26093/cds/vizier.33990795CDSTankosic D.Popovic L.C.Dimitrijevic M.S.2003-03-30T14:35:22Z2003-03-30T14:34:41ZCDS support team

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

cds-question@unistra.fratomic-physicsIn hot star atmospheres, the Stark broadening mechanism is the main pressure broadening mechanism. An interesting application where such a mechanism is of interest is the modeling and investigation of hot star spectra, stellar atmospheres and subphotospheric layers. Consequently, for the investigation and modeling of the Hg-Mn star and other type of hot star atmospheres, the Stark broadening parameters for Co III spectral lines may be of interest. Here we present Stark broadening data for 20 Co III spectral lines (from a^6^D-z^6^D^o^ and a^6^D-z^6^F^o^ Co III multiplets), as a function of temperature, calculated by using the modified semi-empirical approach. The importance of the electron-impact effect in the case of the Co III 194.98nm line for several stellar atmosphere models has been tested.2003A&A...399..795Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/399/795CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/365/656 : Zr II & III electron-impact broadening (Popovic+, 2001)VI/98 : Stark broadening of H lines (Stehle+, 1999)J/A+AS/102/607 : Stark widths of FeII lines (Puric+ 1993)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 X. (Dimitrijevic+, 1994)J/A+AS/109/551 : Stark broadening. XII. OIV + OV (Dimitrijevic+, 1995)J/A+AS/113/579 : Stark broadening (Shoening+, 1995)J/A+AS/115/351 : Stark broadening. XIII. C V and P V (Dimitrijevic+, 1996)J/A+AS/116/359 : Xe II lines Stark broadening (Popovic+, 1996)J/A+AS/117/127 : Solar MgI lines Stark broadening (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/120/373 : Sc II, Y II + Zr II Stark width (Popovic+ 1996)J/A+AS/122/163 : Ba I + Ba II Stark broadening (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 : Si XI + Si XIII lines Stark broadening (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 of 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)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/399/795https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/399/795http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/399/795https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/399/795https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/399/795http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/399/795GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/399/795/table1Electron-impact broadening parameters for Co IIIrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransTransitionmeta.id;phys.atmol.transitionlambda1First wavelength0.1nmem.wlfloatlambda2? Second wavelength0.1nmem.wlfloatnullablelambda3? Third wavelength0.1nmem.wlfloatnullableTempTemperaturesKphys.temperatureintFWHMFWHM for electron impacts (1)nmspect.line.widthdoubledshift for electron impacts (2)nmspect.line.broad.Starkdouble