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<ri:Resource created="2019-11-08T13:28:08Z" status="active" updated="2025-06-13T15:25:00Z" 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>ALMA 1.3mm continuum flux measurement of C1-S core</title><shortName>J/ApJ/867/94</shortName><identifier>ivo://CDS.VizieR/J/ApJ/867/94</identifier><altIdentifier>doi:10.26093/cds/vizier.18670094</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kong S.</name></creator><creator><name>Tan J.C.</name></creator><creator><name>Caselli P.</name></creator><creator><name>Fontani F.</name></creator><creator><name>Wang K.</name></creator><creator><name>Butler M.J.</name></creator><date role="Updated">2019-11-08T12:37:45Z</date><date role="Created">2019-11-08T13:28:08Z</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>interstellar-medium</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We present high-resolution (0.2", 1000au) 1.3mm ALMA observations of the massive infrared dark cloud clump, G028.37+00.07-C1, thought to harbor the early stages of massive star formation. Using N_2_D^+^(3-2), we resolve the previously identified C1-S core, separating the bulk of its emission from two nearby protostellar sources. C1-S is thus identified as a massive (~50M_{sun}_), compact (~0.1pc diameter) starless core, e.g., with no signs of outflow activity. Being highly deuterated, this is a promising candidate for a pre-stellar core on the verge of collapse. An analysis of its dynamical state indicates a sub-virial velocity dispersion compared to a trans-Alfvenic turbulent core model. However, virial equilibrium could be achieved with sub- Alfvenic conditions involving magnetic field strengths of ~2mG.</description><source format="bibcode">2018ApJ...867...94K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/867/94</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/J/A+A/291/943">J/A+A/291/943 : Protostellar cores (Ossenkopf+, 1994)</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/175/509">J/ApJS/175/509 : Ammonia spectral atlas in Perseus (Rosolowsky+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A51">J/A+A/570/A51 : Molecular lines in 4 IRCS clumps (Shipman+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/592/A21">J/A+A/592/A21 : Are infrared dark clouds really quiescent? (Feng+, 2016)</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/867/94</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/867/94</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/867/94</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/867/94</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/867/94</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/867/94</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><spectral>1.528037907652962e-22 1.528037907652962e-22</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/867/94/table2</name><description>Continuum flux measurement data for Figures 4 and 5</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>RC1-sa</name><description>[588/4193]? Projected radius for C1-Sa annuli</description><unit>AU</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>FC1-sa</name><description>[231/2266]? C1-Sa annulus 1.3mm continuum flux density</description><unit>MJy/sr</unit><ucd>phot.flux.density;em.mm.200-400GHz;spect.continuum</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_FC1-sa</name><description>[10/25]? Uncertainty in FC1-Sa</description><unit>MJy/sr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RC1-So</name><description>[554/8954] Projected radius for C1-S outer annuli</description><unit>AU</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FC1-So</name><description>[79/152] C1-S outer annulus 1.3mm continuum flux density</description><unit>MJy/sr</unit><ucd>phot.flux.density;em.mm.200-400GHz;spect.continuum</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FC1-So</name><description>[7/27] Uncertainty in FC1-So</description><unit>MJy/sr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FC1-Sos</name><description>[46/118] C1-S outer with envelope subtraction annulus 1.3 mm continuum flux density</description><unit>MJy/sr</unit><ucd>phot.flux.density;em.mm.200-400GHz;spect.continuum</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FC1-Sos</name><description>[25/37] Uncertainty in FC1-Sos</description><unit>MJy/sr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>