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<ri:Resource created="2012-08-29T11:10:30Z" 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>Deep NIR survey of the Pipe Nebula. II.</title><shortName>J/ApJ/725/2232</shortName><identifier>ivo://CDS.VizieR/J/ApJ/725/2232</identifier><altIdentifier>doi:10.26093/cds/vizier.17252232</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Roman-Zuniga C.G.</name></creator><creator><name>Alves J.F.</name></creator><creator><name>Lada C.J.</name></creator><creator><name>Lombardi M.</name></creator><date role="Updated">2017-10-16T14:58:06Z</date><date role="Created">2012-08-29T11:10:30Z</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>extinction</subject><subject>interstellar-medium</subject><subject>molecular-clouds</subject><subject>surveys</subject><subject>apparent-magnitude</subject><subject>infrared-sources</subject><description>We present a new set of high-resolution dust extinction maps of the nearby and essentially starless Pipe Nebula molecular cloud. The maps were constructed from a concerted deep near-infrared imaging survey with the ESO-VLT, ESO-NTT, CAHA 3.5m telescopes, and 2MASS data. The new maps have a resolution three times higher than the previous extinction map of this cloud by Lombardi et al. (2006A&amp;A...454..781L) and are able to resolve structures down to 2600AU. We detect 244 significant extinction peaks across the cloud. These peaks have masses between 0.1 and 18.4M_{sun}_, diameters between 1.2 and 5.7x10^4^AU (0.06 and 0.28pc), and mean densities of about 10^4^cm^-3^, all in good agreement with previous results. From the analysis of the mean surface density of companions we find a well-defined scale near 1.4x10^4^AU below which we detect a significant decrease in structure of the cloud. This scale is smaller than the Jeans length calculated from the mean density of the peaks. The surface density of peaks is not uniform but instead it displays clustering. Extinction peaks in the Pipe Nebula appear to have a spatial distribution similar to the stars in Taurus, suggesting that the spatial distribution of stars evolves directly from the primordial spatial distribution of high-density material.</description><source format="bibcode">2010ApJ...725.2232R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/725/2232</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/B/eso">B/eso : ESO Science Archive Catalog (ESO, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/742">J/ApJ/699/742 : Properties of cores in the Pipe Nebula (Rathborne+, 2009)</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/725/2232</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/725/2232</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/725/2232</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/725/2232</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/725/2232</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/725/2232</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/725/2232/table2 (CLUMPFIND-2D identifications in high-resolution extinction maps of the Pipe Nebula)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/725/2232/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/725/2232/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/725/2232/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>258.625</ra><dec>-27.4833</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/725/2232/tablea1 (Near-infrared observations of Pipe Nebula fields)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/725/2232/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/725/2232/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/725/2232/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>257.63157306</ra><dec>-27.42657806</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/28859 28862 28863 29187 29189 29190 29191 29192 29193 29200 29201 29204 29205 29206 29209 29211 29212 29214 29215 29248</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/725/2232?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/725/2232/table2</name><description>CLUMPFIND-2D identifications in high-resolution extinction maps of the Pipe Nebula</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>Reg</name><description>Region name (Stem, Shank, Bowl or Smoke maps, see figure 2)</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>PID</name><description>Peak identification from RLA09 ([R/N]NNN) (1)</description><ucd>meta.id;stat.max</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>m_PID</name><description>[a-h] close peaks (2)</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>n_PID</name><description>[*] Note on PID (3)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Av</name><description>Maximum extinction (4)</description><unit>mag</unit><ucd>phys.absorption;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Req</name><description>[0.022/0.146] Equivalent radius of the peak</description><unit>pc</unit><ucd>phys.size.radius;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[0.054/4.812] Mass of the extinction peak region</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n</name><description>[0.41/4.687] Average density of the peak</description><unit>10000cm**-3</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Simbad column added by the CDS</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>_DE</name><description>Simbad column added by the CDS</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column></table><table><name>J/ApJ/725/2232/tablea1</name><description>Near-infrared observations of Pipe Nebula fields</description><column><name>Field</name><description>Field identification</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Date</name><description>Date of observation</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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