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<ri:Resource created="2018-09-11T10:31:35Z" 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>CH_3_OCH_2_OH ALMA detection in NGC 6334I</title><shortName>J/ApJ/851/L46</shortName><identifier>ivo://CDS.VizieR/J/ApJ/851/L46</identifier><altIdentifier>doi:10.26093/cds/vizier.18519046</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>McGuire B.A.</name></creator><creator><name>Shingledecker C.N.</name></creator><creator><name>Willis E.R.</name></creator><creator><name>Burkhardt A.M.</name></creator><creator><name>El-Abd S.,Motiyenko R.A.</name></creator><creator><name>Brogan C.L.</name></creator><creator><name>Hunter T.R.</name></creator><creator><name>Margules L.</name></creator><creator><name>Guillemin J.-C.,Garrod R.T.</name></creator><creator><name>Herbst E.</name></creator><creator><name>Remijan A.J.</name></creator><date role="Updated">2018-10-09T09:02:39Z</date><date role="Created">2018-09-11T10:31:35Z</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><subject>interstellar-medium</subject><subject>molecular-physics</subject><subject>radio-spectroscopy</subject><description>We report the detection of interstellar methoxymethanol (CH_3_OCH_2_OH) in Atacama Large Millimeter/submillimeter Array (ALMA) Bands 6 and 7 toward the MM1 core in the high-mass star-forming region NGC 6334I at ~0.1-1" spatial resolution. A column density of 4(2)x10^18^cm^-2^ at T_ex_=200K is derived toward MM1, ~34 times less abundant than methanol (CH_3_OH), and significantly higher than predicted by astrochemical models. Probable formation and destruction pathways are discussed, primarily through the reaction of the CH_3_OH photodissociation products, the methoxy (CH_3_O) and hydroxymethyl (CH_2_OH) radicals. Finally, we comment on the implications of these mechanisms on gas-phase versus grain-surface routes operative in the region, and the possibility of electron-induced dissociation of CH3OH rather than photodissociation.</description><source format="bibcode">2017ApJ...851L..46M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/851/L46</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/ApJ/783/130">J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A49">J/A+A/601/A49 : CH_3_NHCHO rotational spectroscopy (Belloche+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/605/L3">J/A+A/605/L3 : SOLIS. I. L1157-B1 NH_2_CHO image (Codella+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/835/46">J/ApJ/835/46 : methoxy radical (CH_3_O) rotational spectrum (Laas+, 2017)</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/ApJ/851/L46</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/851/L46</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/851/L46</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/851/L46</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/851/L46</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/851/L46</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"/><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/851/L46/table2</name><description>Line parameters of CH_3_OCH_2_OH</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>QN</name><description>Quantum numbers</description><ucd>phys.atmol.qn</ucd></column><column><name>Freq</name><description>[239256/351903] Frequency (MHz)</description><unit>MHz</unit><ucd>em.freq;em.mm.200-400GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Siju2</name><description>[0/2] Strength (Debye^2^)</description><unit>D**2</unit><ucd>phys.atmol.collStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Eu</name><description>[31.6/1883] Upper energy (K)</description><unit>K</unit><ucd>phys.energy;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>