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<ri:Resource created="2023-07-31T07:54:58Z" 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>Discovery in space and in laboratory of H2CCCN</title><shortName>J/A+A/676/L5</shortName><identifier>ivo://CDS.VizieR/J/A+A/676/L5</identifier><altIdentifier>doi:10.26093/cds/vizier.36769005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cabezas C.</name></creator><creator><name>Tang J.</name></creator><creator><name>Agundez M.</name></creator><creator><name>Seiki K.</name></creator><creator><name>Sumiyoshi Y.</name></creator><creator><name>Ohshima Y.,Tercero B.</name></creator><creator><name>Marcelino N.</name></creator><creator><name>Fuentetaja R.</name></creator><creator><name>de Vicente P.</name></creator><creator><name>Endo Y.,Cernicharo J.</name></creator><date role="Updated">2024-11-28T20:04:59Z</date><date role="Created">2023-07-31T07:54:58Z</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>We report the first laboratory and interstellar detection of the alpha-cyano vinyl radical (H_2_CCCN). This species was produced in the laboratory by an electric discharge of a gas mixture of vinyl cyanide, CH_2_CHCN, and Ne, and its rotational spectrum was characterized using a Balle-Flygare narrowband-type Fourier-transform microwave spectrometer operating in the frequency region of 8-40GHz. The observed spectrum shows a complex structure due to tunneling splittings between two torsional sublevels of the ground vibronic state, 0+ and 0-, derived from a large-amplitude inversion motion. In addition, the presence of two equivalent hydrogen nuclei makes necessary to discern between ortho- and para-H_2_CCCN. A least squares analysis reproduces the observed transition frequencies with a standard deviation of ca. 3kHz. Using the laboratory predictions, this radical is detected in the cold dark cloud TMC-1 using the Yebes 40m telescope and the QUIJOTE line survey. The 404-303 and 505-404 rotational transitions, composed of several hyperfine components, were observed in the 31.0-50.4GHz range. Adopting a rotational temperature of 6K we derive a column density of (1.4+/-0.2)*10^-11^cm^-2^ and (1.1+/-0.2)*10^-11^cm^-2^ for ortho-H_2_CCCN and para-H_2_CCCN, respectively. The reactions C + CH_3_CN, and perhaps also N + CH_2_CCH, emerge as the most likely routes to H_2_CCCN in TMC-1.</description><source format="bibcode">2023A&amp;A...676L...5C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/676/L5</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/676/L5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/676/L5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/676/L5</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/676/L5</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/676/L5</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/676/L5</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/676/L5/tablea3</name><description>Predicted frequencies for ortho-H_2_C_3_N</description><column><name>Freq</name><description>Frequency</description><unit>MHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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