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<ri:Resource created="2006-09-10T14:48:33Z" 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>Velocity and distance of methanol maser sources</title><shortName>J/other/ChJAA/3.</shortName><identifier>ivo://CDS.VizieR/J/other/ChJAA/3.49</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Xu Y.</name></creator><creator><name>Zheng X.-W.</name></creator><creator><name>Jiang D.-R.</name></creator><date role="Updated">2012-11-13T13:18:13Z</date><date role="Created">2006-09-10T14:48:33Z</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><subject>stellar-distance</subject><description>We present a statistical analysis of 482 6.7GHz methanol maser sources from the available literature, on their maser emission and the characteristics of their associated infrared sources. On the color-color diagram, more than 70% of the objects fall within a very small region (0.57&lt;=[25-12]&lt;=1.30 and 1.30&lt;=[60-12]&lt;=2.50). This suggests that 6.7GHz methanol maser emission occurs only within a very short evolutionary phase during the earliest stage of star formation. The velocity ranges of the masers belong to two main groups: one from 1 to 10km/s, and one from about 11 to 20km/s. These velocity ranges indicate that the masers are probably associated with both disks and outflows. The correlations between the maser and infrared flux densities, and between the maser and infrared luminosities, suggest that far-infrared radiation is a possible pumping mechanism for the masers which most probably originate from some outer molecular envelopes or disks.</description><source format="bibcode">2003ChJAA...3...49X</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/ChJAA/3.49</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/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/AZh/72/22">J/AZh/72/22 : A 95 GHz Survey of Methanol Masers (Valtts+, 1995)</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+AS/143/269">J/A+AS/143/269 : 6.7GHz methanol maser emission survey (Szymczak+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/403/1095">J/A+A/403/1095 : 6.7GHz methanol masers survey of low-mass YSO (Minier+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/410/597">J/A+A/410/597 : Warm dust near methanol masers (Walsh+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/413/233">J/A+A/413/233 : 12.2 GHz methanol survey (Blaszkiewicz+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/428/1019">J/A+A/428/1019 : Rest frequencies of methanol maser lines (Mueller+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/434/613">J/A+A/434/613 : Water maser survey of methanol masers (Szymczak+ 2005)</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><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></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/other/ChJAA/3.49</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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