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<ri:Resource created="2021-07-29T12:01:44Z" status="active" updated="2025-06-13T15:25:00Z" 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>Survey of SiO maser emission in oxygen-rich stars</title><shortName>J/ApJS/253/44</shortName><identifier>ivo://CDS.VizieR/J/ApJS/253/44</identifier><altIdentifier>doi:10.26093/cds/vizier.22530044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rizzo J.R.</name></creator><creator><name>Cernicharo J.</name></creator><creator><name>Garcia-Miro C.</name></creator><date role="Updated">2022-03-01T12:16:35Z</date><date role="Created">2021-07-29T12:01:44Z</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>giant-stars</subject><subject>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>interstellar-medium</subject><subject>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><subject>radio-sources</subject><description>Circumstellar environments of oxygen-rich stars are among the strongest SiO maser emitters. Physical processes such as collisions, infrared pumping, and overlaps favor the inversion of level population and produce maser emission at different vibrational states. Despite numerous observational and theoretical efforts, we still do not have a unified picture including all of the physical processes involved in SiO maser emission. The aim of this work is to provide homogeneous data in a large sample of oxygen-rich stars. We present a survey of 67 oxygen-rich stars from 7 to 1mm, in their rotational transitions from J=1-0 to J=5-4, for vibrational numbers v from 0 to 6 in the three main SiO isotopologs. We have used one of the 34 m NASA antennas at Robledo and the IRAM 30m radio telescope. The first tentative detection of a v=6 line is reported, as well as the detection of new maser lines. The highest vibrational levels seem confined to small volumes, presumably close to the stars. The J=1-0, v=2 line flux is greater than the corresponding v=1 in almost half of the sample, which may confirm a predicted dependence on the pulsation cycle. This database is potentially useful in models which should consider most of the physical agents, time dependency, and mass-loss rates. As a by-product, we report detections of 27 thermal rotational lines from other molecules, including isotopologs of SiS, H_2_S, SO, SO_2_, and NaCl.</description><source format="bibcode">2021ApJS..253...44R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/253/44</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+A/285/247">J/A+A/285/247 : Molecules in O- and C-rich envelopes (Bujarrabal+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/329/219">J/A+A/329/219 : 28SiO in O-rich evolved stars (Pardo+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/470/191">J/A+A/470/191 : Mid-IR and radio interferometry of S Ori (Wittkowski+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/348">J/ApJS/190/348 : 1mm spectral survey of IRC+10216 &amp; VY CMa (Tenenbaum+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/149">J/ApJ/728/149 : Polarized SiO masers of VX Sgr (Vlemmings+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/81">J/ApJ/794/81 : Maser and IR studies of oxygen-rich AGB stars (Yung+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/592/A76">J/A+A/592/A76 : VY CMa ALMA NaCl images (Decin+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/1963">J/MNRAS/466/1963 : Silicate in O-rich evolved stars (Liu+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/597/A25">J/A+A/597/A25 : IK Tau millimeter IRAM-30m line survey (Velilla Prieto+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/615/A8">J/A+A/615/A8 : APEX spectrum of R Dor (159.0-368.5GHz) (De Beck+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/641/A57">J/A+A/641/A57 : Oxygen-rich AGB IRAM spectra (Massalkhi+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/642/A213">J/A+A/642/A213 : SiO maser emission in evolved stars (Gomez-Garrido+, 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/ApJS/253/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/253/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/253/44</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/253/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/253/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/253/44</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/ApJS/253/44/stars (List of observed stars; 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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>Seq</name><description>[1/458] Internal index identifier</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Source</name><description>Source identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>VLSR</name><description>[-70/58] Local Standard of Rest velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Date</name><description>Observation date in 2012; mm-dd</description><ucd>time.epoch;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Trans</name><description>The J-&gt;J-1 transition</description><ucd>phot.color;phys.atmol.transition</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>f_Trans</name><description>[ef] Flag on Trans (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Mode</name><description>Observation mode (2)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>VSpace</name><description>[0.2/1.3] Velocity spacing</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>tInt</name><description>[1/76] Total integration time</description><unit>min</unit><ucd>time.expo</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>rms</name><description>[0.04/7.4] The 1{sigma} rms value</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pol</name><description>Polarization (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table><table><name>J/ApJS/253/44/table4</name><description>Detections</description><column><name>Source</name><description>Source identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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