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<ri:Resource created="2012-08-20T11:43:26Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Polarization of IRAS 18089-1732</title><shortName>J/ApJ/724/L113</shortName><identifier>ivo://CDS.VizieR/J/ApJ/724/L113</identifier><altIdentifier>doi:10.26093/cds/vizier.17249113</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Beuther H.</name></creator><creator><name>Vlemmings W.H.T.</name></creator><creator><name>Rao R.</name></creator><creator><name>van der Tak F.F.S.</name></creator><date role="Updated">2012-09-08T07:15:10Z</date><date role="Created">2012-08-20T11:43:26Z</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>polarimetry</subject><subject>h-ii-regions</subject><subject>interstellar-medium</subject><description>To characterize the magnetic field structure of the outflow and core region within a prototypical high-mass star-forming region, we analyzed polarized CO(3-2) -for the first time observed with the Submillimeter Array- as well as 880um submillimeter continuum emission from the high-mass outflow/disk system IRAS 18089-1732. Both emission features with polarization degrees at a few percent level indicate that the magnetic field structure is largely aligned with the outflow/jet orientation from small core scales to larger outflow scales. Although quantitative estimates are crude, the analysis indicates that turbulent energy dominates over magnetic energy. The data also suggest a magnetic field strength increase from the lower-density envelope to the higher-density core.</description><source format="bibcode">2010ApJ...724L.113B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/724/L113</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/112">V/112 : Catalog of Star-Forming Regions in the Galaxy (Avedisova, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/225">II/225 : Catalog of Infrared Observations, Edition 5 (Gezari+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/515/A42">J/A+A/515/A42 : Catalog of high extinction clouds (Rygl+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PASA/26.439">J/other/PASA/26.439 : K-band images of star-forming regions (Longmore+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/368/1223">J/MNRAS/368/1223 : SCUBA observations of cold cores (Hill+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/417/115">J/A+A/417/115 : High-mass protostellar candidates (Williams+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/566/945">J/ApJ/566/945 : Massive star forming regions at 1.2mm (Beuther+, 2002)</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/ApJ/724/L113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/724/L113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/724/L113</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/724/L113</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/724/L113</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/724/L113</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/724/L113/table1</name><description>Polarization measurements</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Source</name><description>Observation source ("Dust emission" (880um), "CO(3-2) at 40km/s" or "CO(3-2) at 44km/s")</description><ucd>obs.param</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>oRA</name><description>Offset in Right Ascension from phase center (1)</description><unit>arcsec</unit><ucd>pos.eq.ra;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>oDE</name><description>Offset in Declination from phase center (1)</description><unit>arcsec</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pol</name><description>[1/67] Polarization of Source</description><unit>%</unit><ucd>phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PA</name><description>[-88/89] Polarization angle</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>