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<ri:Resource created="2008-04-20T16:38:10Z" 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>Catalog of Class I methanol masers</title><shortName>J/AZh/84/579</shortName><identifier>ivo://CDS.VizieR/J/AZh/84/579</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Val'tts I.E.</name></creator><creator><name>Larionov G.M.</name></creator><date role="Updated">2017-10-16T14:57:29Z</date><date role="Created">2008-04-20T16:38:10Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>radial-velocity</subject><description>A catalog of class I methanol masers discovered so far in the Southern and Northern hemispheres is presented. The catalog contains 160 sources. A statistical analysis shows that, within 2' of the telescope pointing (which corresponds approximately to the field of view of single antennas used in search surveys), 50% of class I methanol masers are associated with objects characteristic of active starforming regions: IRAS sources, ultracompact HII regions, and dense gas dust clouds, as well as OH and H2O interstellar masers. At the same time, bipolar out flows (which could play an active part in pumping the methanol masers) are associated with fewer than 25% of class I methanol masers. In 72% of cases, class I methanol masers are associated with class II methanol maser sources. These results suggest that methanol maser condensations are more appropriately classified by the transition type (that is, the pumping mechanism) than their association with other astronomical objects.</description><source format="bibcode">2007AZh....84..579V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/84/579</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/J/AZh/71/37">J/AZh/71/37 : Thermal Methanol from 33 Clouds at 48GHz (Slysh+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/72/22">J/AZh/72/22 : A 95GHz Survey of Methanol Masers (Valtts+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/110/81">J/A+AS/110/81 : Methanol masers towards IRAS sources (van der Walt+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/314/615">J/A+A/314/615 : Maps of the 36 GHz methanol emission (Liechti+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/291/261">J/MNRAS/291/261 : Methanol maser of IRAS-selected sources (Walsh+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/134/115">J/A+AS/134/115 : Medicina 6.7GHz methanol masers survey (Slysh+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/432/737">J/A+A/432/737 : 6.7GHz Methanol Masers General Catalogue (Pestalozzi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/414/235">J/A+A/414/235 : OH maser emission from star forming regions (Szymczak+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/359/1498">J/MNRAS/359/1498 : Class I and class II methanol masers (Ellingsen+, 2005)</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/AZh/84/579</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/84/579</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/84/579</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/84/579</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/84/579</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_Seq</name><description>[*] class II maser also observed (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Name</name><description>Source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>RAB1950</name><description>Right ascension (B1950)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEB1950</name><description>Declination (B1950)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Freq</name><description>Detection frequency (36, 44 or 95GHz)</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Fint</name><description>? 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II/125)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>n_IRAS</name><description>[*] non-coincident IRAS source (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>UCHII</name><description>[(yn|) ] Ultra-compact HII flag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>H2O</name><description>[(yn|) ] H2O maser flag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>OH</name><description>[(yn|) ] OH maser flag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CS</name><description>[(yn|) ] CS maser flag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Bflow</name><description>([yn|) ] Bipolar flow flag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Dist</name><description>? Kinematic distance to the star-forming region hosting the observed maser</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist2</name><description>? Second kinematic distance to the star-forming region hosting the observed maser</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_Dist</name><description>? 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