<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2024-02-27T09:22:08Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>3mm &amp; 2mm maps of seven cores in L1495 filament</title><shortName>J/ApJ/927/213</shortName><identifier>ivo://CDS.VizieR/J/ApJ/927/213</identifier><altIdentifier>doi:10.26093/cds/vizier.19270213</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Punanova A.</name></creator><creator><name>Vasyunin A.</name></creator><creator><name>Caselli P.</name></creator><creator><name>Howard A.</name></creator><creator><name>Spezzano S.</name></creator><creator><name>Shirley Y.,Scibelli S.</name></creator><creator><name>Harju J.</name></creator><date role="Updated">2024-11-06T20:23:56Z</date><date role="Created">2024-02-27T09:22:08Z</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>star-forming-regions</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>interstellar-medium</subject><description>Chemical models predict that in cold cores gas-phase methanol is expected to be abundant at the outer edge of the CO depletion zone, where CO is actively adsorbed. CO adsorption correlates with volume density in cold cores, and, in nearby molecular clouds, catastrophic CO freeze-out happens at volume densities above 10^4^cm^-3^. The methanol production rate is maximized there and its freeze-out rate does not overcome its production rate, while the molecules are shielded from UV destruction by gas and dust. Thus, in cold cores, methanol abundance should generally correlate with visual extinction, which depends on both volume and column density. In this work, we test the most basic model prediction that maximum methanol abundance is associated with a local A_V_~4mag in dense cores and constrain the model parameters with the observational data. With the IRAM 30m antenna, we mapped the CH_3_OH(2-1) and (3-2) transitions toward seven dense cores in the L1495 filament in Taurus to measure the methanol abundance. We use the Herschel/SPIRE maps to estimate visual extinction, and the C^18^O(2-1) maps from Tafalla &amp; Hacar to estimate CO depletion. We explored the observed and modeled correlations between the methanol abundances, CO depletion, and visual extinction, varying the key model parameters. The modeling results show that hydrogen surface diffusion via tunneling is crucial to reproduce the observed methanol abundances, and the necessary reactive desorption efficiency matches the one deduced from laboratory experiments.</description><source format="bibcode">2022ApJ...927..213P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/927/213</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/220">VII/220 : Barnard's Catalogue of 349 Dark Objects in the Sky (Barnard, 1927)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/7">VII/7 : Lynds' Catalogue of Dark Nebulae (LDN) (Lynds 1962)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/432/369">J/A+A/432/369 : Leiden Atomic &amp; Molecular Database (LAMDA) (Schoeier+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/259">J/ApJS/186/259 : Taurus Spitzer survey: new candidate members (Rebull+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/554/A55">J/A+A/554/A55 : C^18^O(1-0) and N_2_H^+^(1-0) in L1495/B213 (Hacar+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/786/29">J/ApJ/786/29 : Catalog of distances to molecular clouds (Schlafly+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/574/A104">J/A+A/574/A104 : Dense cores in L1495/B213 complex (Tafalla+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/1008">J/MNRAS/463/1008 : LDN 1495 SCUBA-2 and Herschel data (Ward-Thompson+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/604/A52">J/A+A/604/A52 : B213 filament 150 and 260GHz emission maps (Bracco+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/606/A142">J/A+A/606/A142 : L1544 1.2 and 2mm emission maps (Chacon-Tanarro+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/617/A27">J/A+A/617/A27 : Kinematics of dense gas in L1495 filament (Punanova+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A108">J/A+A/624/A108 : Modeling interstellar sulfur depletion (Laas+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/630/A136">J/A+A/630/A136 : Starless core L1521E chemical structure (Nagy+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/638/A74">J/A+A/638/A74 : Dense cores in Oph molecular cloud (Ladjelate+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A118">J/A+A/633/A118 : 3mm-band study of L183 and L1544 (Lattanzi+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/638/A85">J/A+A/638/A85 : Taurus with Gaia &amp; Herschel (Roccatagliata+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/643/A60">J/A+A/643/A60 : Starless cores CH_3_OH and c-C_3_H_2_ maps (Spezzano+, 2020)</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/927/213</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/927/213</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/927/213</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/927/213</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/927/213</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/927/213</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/927/213/table1 (The mapped cores)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/927/213/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/927/213/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/927/213/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>64.42644583</ra><dec>28.12524444</dec><sr>0.005555555555555556</sr></testQuery></capability><capability><description>Associated data</description><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/ApJ/927/213</accessURL></interface></capability><coverage><spatial>6/1080 1082 1168</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/927/213?format=ascii</footprint><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/927/213/table1</name><description>The mapped cores</description><column><name>Core</name><description>Name of the dense core in Seo+ 2015ApJ...805..185S ; (&lt;[SSG2015] NN&gt; in Simbad)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Reg</name><description>Region identifier according to Barnard 1927, VII/220 ; (&lt;Barnard NNN&gt; in Simbad)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</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>f_ID</name><description>[*] *: protostellar core</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>[4] Hour of right ascension (J2000) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[26/28] Degree of declination (J2000) (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>fits1</name><description>Download the FITS file for the CH3OH(2-1) line at 96.74GHz (3mm)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>FileName1</name><description>Name of the FITS file in subdirectory "fits" for the CH3OH(2-1) line at 96.74GHz (3mm)</description><ucd>meta.id;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>fits2</name><description>Download the FITS file for the CH3OH(3-2) line at 145.10GHz (2mm)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>FileName2</name><description>Name of the FITS file in subdirectory "fits" for the CH3OH(3-2) line at 145.10GHz (2mm)</description><ucd>meta.id;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>ID</name><description>[1/16]? Identifier of the dense core in Hacar+ 2013, J/A+A/554/A55 ; (&lt;[HTK2013] NN&gt; in Simbad)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>