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<ri:Resource created="2015-04-15T15:00:57Z" 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>Polarization from stars behind IC63 nebula</title><shortName>J/ApJ/775/84</shortName><identifier>ivo://CDS.VizieR/J/ApJ/775/84</identifier><altIdentifier>doi:10.26093/cds/vizier.17750084</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andersson B.-G.</name></creator><creator><name>Piirola V.</name></creator><creator><name>De Buizer J.</name></creator><creator><name>Clemens D.P.</name></creator><creator><name>Uomoto A.,Charcos-Llorens M.</name></creator><creator><name>Geballe T.R.</name></creator><creator><name>Lazarian A.</name></creator><creator><name>Hoang T.</name></creator><creator><name>Vornanen T.</name></creator><date role="Updated">2018-01-04T08:21:22Z</date><date role="Created">2015-04-15T15:00:57Z</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>interstellar-medium</subject><subject>dwarf-stars</subject><subject>h-ii-regions</subject><description>In the interstellar medium (ISM), molecular hydrogen is expected to form almost exclusively on the surfaces of dust grains. Due to that molecule's large formation energy (-4.5eV), several dynamical effects are likely associated with the process, including the alignment of asymmetric dust grains with the ambient magnetic field. Such aligned dust grains are, in turn, believed to cause the broadband optical/infrared polarization observed in the ISM. Here, we present the first observational evidence for grain alignment driven by H_2_ formation, by showing that the polarization of the light from stars behind the reflection nebula IC 63 appears to correlate with the intensity of H_2_ fluorescence. While our results strongly suggest a role for "Purcell rockets" in grain alignment, additional observations are needed to conclusively confirm their role. By showing a direct connection between H_2_ formation and a probe of the dust characteristics, these results also provide one of the first direct confirmations of the grain-surface formation of H_2_. We compare our observations to ab initio modeling based on Radiative Torque Alignment (RAT) theory.</description><source format="bibcode">2013ApJ...775...84A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/775/84</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/239">I/239 : The Hipparcos and Tycho Catalogues (ESA 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2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/470/161">J/A+A/470/161 : UBV photometry of HII regions exciting stars (Russeil+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/448/411">J/A+A/448/411 : The DRAO polarization survey (Wolleben+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/873">J/AJ/130/873 : Properties of BQS objects in the SDSS DR3 area (Jester+, 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/ApJ/775/84</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/775/84</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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