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<ri:Resource created="2020-03-09T07:11:36Z" 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>Plasma environment effects on Fe IX-XVI K lines</title><shortName>J/A+A/635/A70</shortName><identifier>ivo://CDS.VizieR/J/A+A/635/A70</identifier><altIdentifier>doi:10.26093/cds/vizier.36350070</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Deprince J.</name></creator><creator><name>Bautista M.A.</name></creator><creator><name>Fritzsche S.</name></creator><creator><name>Garcia J.</name></creator><creator><name>Kallman T.,Mendoza C.</name></creator><creator><name>Palmeri P.</name></creator><creator><name>Quinet P.</name></creator><date role="Updated">2020-05-05T12:40:07Z</date><date role="Created">2020-03-09T07:11:36Z</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>In the context of black-hole accretion disks, we have computed plasma environment effects on the atomic parameters used to model the decay of K-vacancy states in moderately charged iron ions, namely FeIX-FeXVI. We use the fully relativistic multiconfiguration Dirac-Fock (MCDF) method approximating the plasma electron-nucleus and electron-electron screenings with a time-averaged Debye-Huckel potential. Modified ionization potentials, K thresholds, wavelengths, radiative emission rates and Auger widths are reported for astrophysical plasmas characterized by electron temperatures and densities respectively in the ranges 10^5^-10^7^K and 10^18^-10^22^cm^-3^. This study confirms that the high-resolution X-ray spectrometers onboard the future XRISM and ATHENA space missions could detect the lowering of the K edges of these ions due to the extreme plasma conditions occurring in accretion disks around compact objects.</description><source format="bibcode">2020A&amp;A...635A..70D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/635/A70</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/635/A70</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/635/A70</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/635/A70</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/635/A70</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/635/A70</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/635/A70</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/635/A70/table5</name><description>Wavelengths and Transition probabilities</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>Zeff</name><description>Effective charge</description><ucd>phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Trans</name><description>Transition identification</description><ucd>meta.id;phys.atmol.transProb;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType" arraysize="39*">char</dataType></column><column><name>WL1</name><description>Wavelength in Angstrom (mu=0a.u.)</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WL2</name><description>Wavelength in Angstrom (mu=0.1a.u.)</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WL3</name><description>Wavelength in Angstrom (mu=0.25a.u.)</description><unit>0.1nm</unit><ucd>em.wl;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ar1</name><description>Transition probability (mu=0a.u.)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ar2</name><description>Transition probability (mu=0.1a.u.)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ar3</name><description>Transition probability (mu=0.25a.u.)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/635/A70/table6</name><description>Auger widths</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>Zeff</name><description>Effective charge</description><ucd>phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Lev</name><description>K-vacancy level</description><ucd>phys.energy;phys.atmol.level</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>Aa1</name><description>Auger width (mu=0a.u.)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Aa2</name><description>Auger width (mu=0.1a.u.)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Aa3</name><description>Auger width (mu=0.25a.u.)</description><unit>s**-1</unit><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>