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<ri:Resource created="2022-07-19T08:54:57Z" 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>2mm and 3mm sp. of CRL 2688 protoplanetary nebula</title><shortName>J/ApJS/259/56</shortName><identifier>ivo://CDS.VizieR/J/ApJS/259/56</identifier><altIdentifier>doi:10.26093/cds/vizier.22590056</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Qiu J.-J.</name></creator><creator><name>Zhang Y.</name></creator><creator><name>Zhang J.-S.</name></creator><creator><name>Nakashima J.-I.</name></creator><date role="Updated">2022-08-26T08:05:20Z</date><date role="Created">2022-07-19T08:54:57Z</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>planetary-nebulae</subject><subject>radio-spectroscopy</subject><description>We present observations of the carbon-rich protoplanetary nebula CRL2688 made with the Institut de Radioastronomie Millimetrique 30m telescope in the 3 and 2mm bands. In total, 196 transition lines belonging to 38 molecular species and isotopologues are detected, among which, to the best of our knowledge, 153 transition lines and 13 species are the first reported for this object. Additionally, in order to contribute to future research, we have collected observational data on the molecular lines of CRL 2688 from the literature and compiled them into a single unified catalog. We find that the molecular abundance of CRL 2688 cannot be explained by the standard model of a circumstellar envelope. The implications of metal-bearing molecules on circumstellar chemistry are discussed.</description><source format="bibcode">2022ApJS..259...56Q</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/259/56</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/B/eso">B/eso : ESO Science Archive Catalog (ESO, 1991-2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/139">VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/299/755">J/A+A/299/755 : Stellar evolution. II. 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(Hrivnak+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/17">J/ApJS/193/17 : Spectral-line survey of IRC+10216 at 293-355GHz (Patel+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/574/A56">J/A+A/574/A56 : IRC +10216 17.8GHz-26.3GHz spectrum (Gong+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/606/A74">J/A+A/606/A74 : IRC +10216 13.3GHz-18.5GHz spectrum (Zhang+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A120">J/A+A/633/A120 : SgrB2(M) ^13^CCC and C^13^CC spectra (Giesen +, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/634/A125">J/A+A/634/A125 : NGC 1068 nucleus molecular line spectra at 2mm (Qiu+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/162/191">J/AJ/162/191 : 2011-2021 calibrator observations of SCUBA-2 (Mairs+, 2021)</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/ApJS/259/56</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/259/56</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/259/56</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/259/56</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/259/56</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/259/56</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/ApJS/259/56/fig1</name><description>The full spectra of CRL 2688 obtained in current observations</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>Freq</name><description>[75.7/184.3] Rest frequency</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tmb</name><description>[-0.25/11.8] Main beam temperature (1)</description><unit>K</unit><ucd>phys.temperature</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>