J/A+AS/127/295ivo://CDS.VizieR/J/A+AS/127/295CDSPopovic L.C.Dimitrijevic M.S.1998-02-04T11:20:43Z1998-02-04T12:20:37ZCDS support team

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

cds-question@unistra.fratomic-physicsWith the development of space-borne spectroscopy, spectral line parameters for a large number of lines become of increasing interest for astrophysics. To provide Stark broadening data for ion lines from complex spectra, we present here calculated Stark widths for 37 Kr II lines from the 5s-5p transition. The calculations were performed by using a modified semiempirical approach. The obtained Stark widths are on average in satisfactory agreement with available experimental data.1998A&AS..127..295Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/127/295CatalogResearchIsServedByTAP VizieR generic servicerelated-toVI/98 : Stark broadening of H lines (Stehle+, 1999)J/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/127/543 : 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)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+AS/127/295https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/127/295http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/127/295https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/127/295https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/127/295http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/127/295GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/127/295/table1*Stark full widths (FWHM) of Kr II spectral linesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransTransitionmeta.id;phys.atmol.transitioncharLambdaWavelengthnmem.wlfloatTTemperatureKphys.temperatureintWStark widthnmspect.line.broad.StarkdoubleJ/A+AS/127/295/table2*Comparison of theoretical Stark widths (w_th_ - FWHM) with experimental datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransTransitionmeta.id;phys.atmol.transitioncharLambdaWavelengthnmem.wlfloatTTemperature1000Kphys.temperaturefloatWmMeasured Stark widthnmspect.line.broad.StarkfloatWm/WthMeasured to theoretical Stark widths ratiostat.fit.omcfloatrefReference for theoretical Stark width (1)meta.refint