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<ri:Resource created="2010-05-31T20:28:36Z" 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>JHK' photometry of M17 silhouette object</title><shortName>J/ApJ/672/398</shortName><identifier>ivo://CDS.VizieR/J/ApJ/672/398</identifier><altIdentifier>doi:10.26093/cds/vizier.16720398</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ito M.</name></creator><creator><name>Yamashita T.</name></creator><creator><name>Sako S.</name></creator><creator><name>Takami H.</name></creator><creator><name>Hayano Y.</name></creator><creator><name>Terada H.</name></creator><date role="Updated">2017-10-09T13:34:36Z</date><date role="Created">2010-05-31T20:28:36Z</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>open-star-clusters</subject><subject>young-stellar-objects</subject><subject>pre-main-sequence-stars</subject><subject>infrared-photometry</subject><description>To study how the structure of the envelopes of young stellar objects (YSOs) evolve, we carried out a deep JHK'-band imaging survey of the M17 star-forming region using a near-infrared camera and the Infrared Camera and Spectrograph with adaptive optics mounted on the Subaru Telescope. In this survey, we found 51 dark silhouettes against bright near-infrared nebula emissions as background lights. They are regarded as envelopes associated with YSOs due to their size and association with the YSOs. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[IYS2008]</name><description>Designation (JNN, HNN, KNN or NSN) (1)</description><ucd>meta.id;phys.atmol.configuration</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Jmag</name><description>? J magnitude (1.25+/-0.16um)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Hmag</name><description>? 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Mass of the central YSO</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AV</name><description>? Silhouette peak extinction</description><unit>mag</unit><ucd>phys.absorption;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Morph</name><description>Morphology of the silhouette (2)</description><ucd>src.morph.param</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Rad1</name><description>Distance from the extinction peak to the silhouette border</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rad2</name><description>? 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