J/A+A/425/1147ivo://CDS.VizieR/J/A+A/425/1147doi:10.26093/cds/vizier.34251147CDSDimitrijevic M.S.Dacic M.Cvetkovic Z.Simic Z.2004-12-11T20:44:08Z2004-12-11T21:44:01ZCDS support team

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

cds-question@unistra.fratomic-physicsStark broadening of the 18 Ga I transitions has been analyzed within the framework of the semiclassical perturbation method. Results obtained have been compared with available experimental and theoretical data and used for the consideration of the influence of the Stark broadening effect in stellar atmospheres2004A&A...425.1147Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/425/1147CatalogResearchIsServedByTAP 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/423/397 : Si V (Ben Nessib+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/425/1147https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/425/1147http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/425/1147https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/425/1147https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/425/1147http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/425/1147GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/425/1147/table1Stark broadening parameters due to electron-, and proton-impacts for Ga IrecnoRecord number assigned by the VizieR team. Should Not be used for identification.intNPerturber densitycm**-3doubleElElementcharTrTransitioncharlambdaWavelength0.1nmdoubleCParameter C (1)0.1nm.cm**-3doubleTTemperatureKfloatWeFWHM for electron impacts (2)0.1nmdoubledeshift for electron impacts (3)0.1nmdoubleWpFWHM for proton impacts (2)0.1nmdoubledpshift for proton impacts (3)0.1nmdouble