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<ri:Resource created="2012-08-29T17:19:50Z" 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>Chemistry of IRC+10216 inner wind modelled</title><shortName>J/A+A/545/A12</shortName><identifier>ivo://CDS.VizieR/J/A+A/545/A12</identifier><altIdentifier>doi:10.26093/cds/vizier.35450012</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cherchneff I.</name></creator><date role="Updated">2012-11-11T22:14:14Z</date><date role="Created">2012-08-29T17:19:50Z</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>carbon-stars</subject><subject>stellar-evolutionary-models</subject><description>We model the chemistry of the inner wind of the carbon star IRC+10216 and consider the effects of periodic shocks induced by the stellar pulsation on the gas to follow the non-equilibrium chemistry in the shocked gas layers. We consider a very complete set of chemical families, including hydrocarbons and aromatics, hydrides, halogens, and phosphorous-bearing species. Our derived abundances are compared to those for the latest observational data from large surveys and the Herschel telescope. A semi-analytical formalism based on parameterised fluid equations is used to describe the gas density, velocity, and temperature from 1R to 5R. The chemistry is described using a chemical kinetic network of reactions and a set of stiff, ordinary, coupled differential equations is solved.</description><source format="bibcode">2012A&amp;A...545A..12C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/545/A12</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/J/A+A/330/676">J/A+A/330/676 : IRC+10216 Silicon and sulfur chemistry (Willacy+ 1998)</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/545/A12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/545/A12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/545/A12</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/545/A12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/545/A12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/545/A12</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/545/A12/tablea1</name><description>The chemical reaction network ordered by type of reactions</description><column><name>Prod</name><description>Products</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>React</name><description>Reactants</description><ucd>phys.atmol.element</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>n</name><description>n factor</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><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>Code</name><description>[ABCD] Code for type of reaction (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Num</name><description>Reaction number (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>A</name><description>A coefficient (in s^-1^, cm^3^/s or cm^6^/s depending on the type of process)</description><ucd>phys.atmol.transProb</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ea</name><description>Activation energy Ea in Kelvin</description><unit>K</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref</name><description>References for the rate data (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="43*">char</dataType></column></table></schema></tableset></ri:Resource>