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<ri:Resource created="1997-12-09T21:16:54Z" 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>IRAS PSC new OH/IR stars. III.</title><shortName>J/ApJS/89/189</shortName><identifier>ivo://CDS.VizieR/J/ApJS/89/189</identifier><altIdentifier>doi:10.26093/cds/vizier.20890189</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chengalur J.N.</name></creator><creator><name>Lewis B.M.</name></creator><creator><name>Eder J.</name></creator><creator><name>Terzian Y.</name></creator><date role="Updated">2013-03-05T06:38:12Z</date><date role="Created">1997-12-09T21:16:54Z</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>infrared-sources</subject><subject>radio-astronomy</subject><description>We present the results of 1612MHz observations conducted at the Arecibo Observatory of 571 color-selected sources from the IRAS Point Source Catalog. Of these sources we detect 132, 113 for the first time. This is the third part of an Arecibo survey of color-selected IRAS sources. The earlier two parts together detected a total of 268 sources of 1612MHz emission. An analysis of the properties of the OH/IR stars detected in all three parts of the survey is included. In particular we compute the limiting 1612MHz peak flux of the entire survey to be ~40mJy. The correlation between the IRAS infrared fluxes and the 1612MHz flux of the 132 sources detected in part III of the survey is smaller than that found in the earlier parts of the survey. This is to be expected from the intrinsic variability of OH/IR stars and the longer time gap between the 1612MHz observations and the IRAS measurements. We identify a subset of 54 stars as being near the tangent point of the galactic rotation curve. Using the kinematical distances to these stars we find that the efficiency of momentum transfer varies exponentially with the (25-12){mu}m color, consistent with the stellar outflow being driven by radiation pressure. Further the IR pump efficiency increases with increasing optical depth of the circumstellar shell, as expected for radiative pumping. The bolometric luminosity function is found to decrease sharply above L_Bol_=5600L_{sun}_, and the 1612MHz luminosity function shows a corresponding falloff above L_1612_=1.8x10^-8^L_{sun}_. We also find direct confirmation of the expectation that sources with large expansion velocity are more luminous than sources with small expansion velocity.</description><source format="bibcode">1993ApJS...89..189C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/89/189</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/125">II/125 : IRAS Point Source Catalogue, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/90/327">J/A+AS/90/327 : IRAS Point Source 1612MHz OH survey (te Lintel Hekkert+ 1991)</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/89/189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/89/189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/89/189</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/89/189</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/89/189</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/89/189?format=ascii</footprint><waveband>Infrared</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJS/89/189/table1</name><description>Detections</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Integrated 1612MHz flux in the high-velocity half of the spectrum</description><unit>mJy.km/s</unit><ucd>phot.flux.density;em.radio.1500-3000MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>DV(100)</name><description>? Velocity separation between the half-power points of the two peaks in the line profile {DELTA}V_100_</description><unit>km/s</unit><ucd>phys.veloc;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>DV(50)</name><description>? Velocity separation between the half-power points of the two peaks in the line profile {DELTA}V_50_</description><unit>km/s</unit><ucd>phys.veloc;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>u_DV(50)</name><description>[)] Uncertainty flag on DV(50).</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Vl</name><description>LSR velocity of the low-velocity peak</description><unit>km/s</unit><ucd>phys.veloc;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vh</name><description>? LSR velocity of the high-velocity peak</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>&lt;V&gt;</name><description>Systemic LSR velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(25-12)</name><description>? (25-12){mu}m infrared color</description><unit>mag</unit><ucd>phot.color;em.IR.8-15um;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>(60-25)</name><description>? (60-25){mu}m infrared color</description><unit>mag</unit><ucd>phot.color;em.IR.15-30um;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Name</name><description>Other name, if the source corresponds to one known before the IRAS survey</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJS/89/189/table2</name><description>Non-detections</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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