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<ri:Resource created="2014-09-03T13:50:50Z" status="active" updated="2026-03-18T20:01:05Z" 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>Simultaneous SiO and H2O maser observations. IV.</title><shortName>J/AJ/147/22</shortName><identifier>ivo://CDS.VizieR/J/AJ/147/22</identifier><altIdentifier>doi:10.26093/cds/vizier.51470022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kim J.</name></creator><creator><name>Cho S.-H.</name></creator><creator><name>Kim S.J.</name></creator><date role="Updated">2026-03-18T20:01:05Z</date><date role="Created">2014-09-03T13:50:50Z</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>interstellar-masers</subject><subject>variable-stars</subject><subject>radio-astronomy</subject><description>Based on the simultaneous observational results of SiO and H_2_O masers toward 401 evolved stars, we have performed statistical analyses. We find that the peak and integrated intensities of SiO masers are stronger than those of H_2_O masers in both Mira variables and OH/IR stars at most optical phases. However, the relative intensity ratios of H_2_O to SiO masers in OH/IR stars are larger than those in Mira variables. Moreover, the intensity ratios of H_2_O to SiO masers are found to be increased around the optical phases from 0-0.4. The H_2_O photon luminosities also tend to be more dependent on the optical phase compared with those of SiO masers. These facts suggest that H_2_O masers are more sensitive to expanding the motion of circumstellar envelopes and also shock waves arising from the pulsations of the central star compared with SiO masers. This result may also be related to the differences in the maser location and pumping mechanism between H_2_O and SiO masers. The full width at zero power of SiO masers in Mira variables shows similar values to those of OH/IR stars, while those of H_2_ O masers in OH/IR stars show larger values than those of Mira variables. These differences may originate from the different mass-loss rates and the different location of the two masers. The mean velocity shift of SiO and H_2_O masers with respect to the stellar velocity was investigated as a function of optical phase. The velocity shift of the H_2_O masers shows that the redshifted emission dominates during the phases from 0.3-0.6, while the blueshifted emission appears at phase 0.6 and coexists with the redshifted emission during other phases. These features show an associated pattern with the CO {Delta}V=3 radial velocity curve, which exhibits a typical pulsation motion. On the other hand, the velocity shift of the SiO v=2 maser shows slightly similar features to the H_2_O maser, while that of SiO v=1 does not show these similar features. Finally, the distributions of all 401 observed sources are investigated in the IRAS two-color diagram in relation to the late evolutionary processes of asymptotic giant branch stars.</description><source format="bibcode">2014AJ....147...22K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/147/22</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/II/264">II/264 : ASAS Variable Stars in Southern hemisphere (Pojmanski+, 2002-2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/18">V/18 : Catalogue of Late-type Stars with Maser Emission (Engels, 1979)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/22">J/AJ/145/22 : Simultaneous SiO and H2O maser observations (Kim+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/129">J/AJ/144/129 : Properties of 83 known stellar SiO maser sources (Cho+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/64/4">J/PASJ/64/4 : SiO maser survey of nearby red variables (Deguchi+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/669/446">J/ApJ/669/446 : Observations of SiO masers (Nakashima+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/56/765">J/PASJ/56/765 : SiO maser survey of IRAS sources (Deguchi+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/203">J/PASJ/55/203 : SiO maser survey toward inner Galactic disk (Nakashima+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/229">J/PASJ/55/229 : SiO maser survey of cold IRAS sources (Nakashima+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/101/153">J/A+AS/101/153 : Galactic H2O masers (Palagi+ 1993)</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/AJ/147/22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/147/22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/147/22</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/147/22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/147/22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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