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<ri:Resource created="2019-11-04T15:31:07Z" 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>NIR observations of GF 9/LDN 1082C field stars</title><shortName>J/ApJ/867/79</shortName><identifier>ivo://CDS.VizieR/J/ApJ/867/79</identifier><altIdentifier>doi:10.26093/cds/vizier.18670079</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Clemens D.P.</name></creator><creator><name>El-Batal A.M.</name></creator><creator><name>Cerny C.</name></creator><creator><name>Kressy S.</name></creator><creator><name>Schroeder G.</name></creator><creator><name>Pillai T.</name></creator><date role="Updated">2020-03-26T14:18:40Z</date><date role="Created">2019-11-04T15:31:07Z</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>infrared-photometry</subject><subject>molecular-clouds</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>The orientation of the magnetic field (B field) in the filamentary dark cloud GF 9 was traced from the periphery of the cloud into the L1082C dense core that contains the low-mass, low-luminosity Class 0 young stellar object (YSO) GF 9-2 (IRAS 20503+6006). This was done using SOFIA HAWC+ dust thermal emission polarimetry (TEP) at 216{mu}m in combination with Mimir near-infrared background starlight polarimetry (BSP) conducted in the H band (1.6{mu}m) and K band (2.2{mu}m). These observations were augmented with published I-band (0.77{mu}m) BSP and Planck 850{mu}m TEP to probe B-field orientations with offset from the YSO in a range spanning 6000au to 3pc. No strong B-field orientation change with offset was found, indicating remarkable uniformity of the B-field from the cloud edge to the YSO environs. This finding disagrees with weak-field models of cloud core and YSO formation. The continuity of inferred B-field orientations for both TEP and BSP probes is strong evidence that both are sampling a common B field that uniformly threads the cloud, core, and YSO region. Bayesian analysis of Gaia DR2 stars matched to the Mimir BSP stars finds a distance to GF 9 of 270+/-10pc. No strong wavelength dependence of B-field orientation angle was found, contrary to previous claims.</description><source format="bibcode">2018ApJ...867...79C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/867/79</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/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/110/268">J/AJ/110/268 : Red and infrared polarimetry in galactic plane (Creese+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/650/945">J/ApJ/650/945 : Polarisation around dark cloud GF 9 (Poidevin+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/13">J/ApJS/213/13 : Polarization maps of star-forming cores &amp; SFRs (Hull+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/176">J/ApJ/833/176 : The magnetic field of L1544. 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