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<ri:Resource created="2017-11-06T08:58:58Z" 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>IRDC G028.23-00.19 NIR polarimetry analysis</title><shortName>J/ApJ/836/199</shortName><identifier>ivo://CDS.VizieR/J/ApJ/836/199</identifier><altIdentifier>doi:10.26093/cds/vizier.18360199</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hoq S.</name></creator><creator><name>Clemens D.P.</name></creator><creator><name>Guzman A.E.</name></creator><creator><name>Cashman L.R.</name></creator><date role="Updated">2017-12-07T07:15:28Z</date><date role="Created">2017-11-06T08:58:58Z</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>galaxy-kinematics</subject><subject>magnetic-fields</subject><subject>molecular-clouds</subject><description>The importance of the magnetic (B) field in the formation of infrared dark clouds (IRDCs) and massive stars is an ongoing topic of investigation. We studied the plane-of-sky B field for one IRDC, G028.23-00.19, to understand the interaction between the field and the cloud. We used near-IR background starlight polarimetry to probe the B field and performed several observational tests to assess the field importance. The polarimetric data, taken with the Mimir instrument, consisted of H-band and K-band observations, totaling 17160 stellar measurements. We traced the plane-of-sky B-field morphology with respect to the sky-projected cloud elongation. We also found the relationship between the estimated B-field strength and gas volume density, and we computed estimates of the normalized mass-to-magnetic flux ratio. The B-field orientation with respect to the cloud did not show a preferred alignment, but it did exhibit a large-scale pattern. The plane-of-sky B-field strengths ranged from 10 to 165{mu}G, and the B-field strength dependence on density followed a power law with an index consistent with 2/3. The mass-to-magnetic flux ratio also increased as a function of density. The relative orientations and relationship between the B field and density imply that the B field was not dynamically important in the formation of the IRDC. The increase in mass-to-flux ratio as a function of density, though, indicates a dynamically important B field. Therefore, it is unclear whether the B field influenced the formation of G28.23. However, it is likely that the presence of the IRDC changed the local B-field morphology.</description><source format="bibcode">2017ApJ...836..199H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/836/199</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/226">II/226 : Stellar polarization catalogs agglomeration (Heiles, 2000)</relatedResource><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/293">II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/641/389">J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/406">J/ApJS/186/406 : 350um polarimetry from CSO (Dotson+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/1019">J/ApJ/723/1019 : Galactic SFR and gas surface densities (Heiderman+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/21">J/ApJ/741/21 : Polarization of stars in Taurus (Chapman+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/60">J/ApJ/756/60 : A 3mm line survey in 37 IR dark clouds (Sanhueza+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2442">J/MNRAS/424/2442 : Catalog of bubbles from Milky Way Project (Simpson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A45">J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 330&lt;l&lt;21 (Contreras+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/793/126">J/ApJ/793/126 : L204 - 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