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<ri:Resource created="2014-01-23T08:03:19Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>HeI lines Stark broadening</title><shortName>J/A+A/561/A135</shortName><identifier>ivo://CDS.VizieR/J/A+A/561/A135</identifier><altIdentifier>doi:10.26093/cds/vizier.35610135</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gigosos M.A.</name></creator><creator><name>Djurovic S.</name></creator><creator><name>Savic I.</name></creator><creator><name>Gonalez-Herrero D.</name></creator><creator><name>Mijatovic Z.,Kovilarov R.</name></creator><date role="Updated">2014-07-05T14:47:17Z</date><date role="Created">2014-01-23T08:03:19Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>atomic-physics</subject><description>The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 587.6, and 706.5nm from neutral helium in plasmas are studied theoretically and experimentally. The aim of this work is to provide information about the connection between the shape and width of spectral lines and the electron density and temperature to be used as a diagnostic tool. The theoretical calculations were carried out through molecular dynamics computer simulations with noninteracting particles. The experimental measurements were done in a plasma of pure helium generated in an electromagnetically driven T-tube. The plasma diagnostics used previous results about the Stark broadening of the HeI 447.1nm and HeI 492.2nm lines and the coherence between the shape of these spectra and those obtained here. The electron temperature was obtained through a Boltzmann-plot of eight lines of SiII.</description><source format="bibcode">2014A&amp;A...561A.135G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/561/A135</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VI/82">VI/82 : Stark broadening of H lines (Stehle 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/98">VI/98 : Stark broadening of H lines (Stehle+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/170/251">J/ApJS/170/251 : Multiplet table for neutral helium (Drake+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/542/A75">J/A+A/542/A75 : Stark broadening for the HeI 492.2 line (Lara+, 2012)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/561/A135</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/561/A135</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/561/A135</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/561/A135</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/561/A135</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/561/A135</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/></coverage><tableset><schema><name>default</name><table><name>J/A+A/561/A135/tables</name><description>Full Width at Half Maximum and Peak Shift of HeI lines (tables 6-29 of the paper)</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>[3889/7281] Wavelength in Angstroms (1)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>mu</name><description>[0.8/10] Reduced mass of the pair emitter-ionic perturber, in proton mass unit (values 0.8, 2, 4, 10)</description><unit>mp</unit><ucd>phys.atmol</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ne</name><description>[1.e21/1.e24] Electron density</description><unit>m**-3</unit><ucd>phys.density;phys.electron</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWHM5</name><description>FWHM of HeI line at T=5000K</description><unit>nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Shift5</name><description>Shift of HeI line at T=5000K</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FWHM10</name><description>FWHM of HeI line at T=10000K</description><unit>nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Shift10</name><description>Shift of HeI line at T=10000K</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FWHM20</name><description>FWHM of HeI line at T=20000K</description><unit>nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Shift20</name><description>Shift of HeI line at T=20000K</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FWHM30</name><description>FWHM of HeI line at T=30000K</description><unit>nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Shift30</name><description>Shift of HeI line at T=30000K</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FWHM40</name><description>FWHM of HeI line at T=40000K</description><unit>nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Shift40</name><description>Shift of HeI line at T=40000K</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FWHM60</name><description>FWHM of HeI line at T=60000K</description><unit>nm</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Shift60</name><description>Shift of HeI line at T=60000K</description><unit>nm</unit><ucd>spect.line.broad.Stark</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>