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<ri:Resource created="2010-10-17T15:24:28Z" 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>Xray properties of protostars in ONC</title><shortName>J/ApJ/677/401</shortName><identifier>ivo://CDS.VizieR/J/ApJ/677/401</identifier><altIdentifier>doi:10.26093/cds/vizier.16770401</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Prisinzano L.</name></creator><creator><name>Micela G.</name></creator><creator><name>Flaccomio E.</name></creator><creator><name>Stauffer J.R.</name></creator><creator><name>Megeath T.,Rebull L.</name></creator><creator><name>Robberto M.</name></creator><creator><name>Smith K.</name></creator><creator><name>Feigelson E.D.</name></creator><creator><name>Grosso N.</name></creator><creator><name>Wolk S.</name></creator><date role="Updated">2017-07-11T13:09:12Z</date><date role="Created">2010-10-17T15:24:28Z</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>young-stellar-objects</subject><subject>x-ray-sources</subject><subject>infrared-photometry</subject><subject>astronomical-object-identification</subject><subject>open-star-clusters</subject><description>The origin and evolution of the X-ray emission in very young stellar objects (YSOs) are not yet well understood because it is very hard to observe YSOs in the protostellar phase. Using COUP data, we study the X-ray properties of stars in the ONC in different evolutionary classes: luminosities, hydrogen column densities N_H_, effective plasma temperatures, and time variability are compared to understand if the interaction between the circumstellar material and the central object can influence the X-ray emission. We have assembled the deepest and most complete photometric catalog of objects in the ONC region from the UV to 8um using data from the HST Treasury Program; deep and almost simultaneous UBVI and JHK images taken, respectively, with WFI at ESO 2.2m and ISPI at CTIO 4m telescopes; and Spitzer IRAC imaging. We select high-probability candidate Class 0-I protostars, a sample of "bona fide" Class II stars, and a set of Class III stars with IR emission consistent with normal photospheres. Our principal result is that Class 0-Ia objects are significantly less luminous in X-rays, in both the total and hard bands, than the more evolved Class II stars with mass larger than 0.5M_{sun}_; the latter show X-ray luminosities similar to those of Class 0-Ib stars.</description><source format="bibcode">2008ApJ...677..401P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/677/401</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/J/ApJ/574/258">J/ApJ/574/258 : X-ray-emitting young stars in the Orion nebula (Feigelson+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/582/382">J/ApJ/582/382 : Chandra X-ray sources in Orion Nebula Cluster (Flaccomio+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/584/911">J/ApJ/584/911 : X-rays in the Orion nebula cluster (Feigelson+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1763">J/AJ/130/1763 : 11.7{mu}m point sources in Orion (Smith+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/1534">J/AJ/129/1534 : Mid-IR photometry in the Orion Nebula (Robberto+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/160/319">J/ApJS/160/319 : COUP: observations and source lists (Getman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/160/450">J/ApJS/160/450 : X-ray emission in Orion Nebula young stars (Flaccomio+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/704">J/ApJ/660/704 : Optical and X-ray variability of ONC PMS (Stassun+, 2007)</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/677/401</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/677/401</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/677/401</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/677/401</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/677/401</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/677/401</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/677/401/NIRphot (Combined table from original tables)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/677/401/NIRphot?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/677/401/NIRphot?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/677/401/NIRphot?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>83.7093162</ra><dec>-5.3641575</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/21438 21439 22804 22805</spatial><spectral>2.0616683193919197e-20 1.7003137259100215e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/677/401?format=ascii</footprint><waveband>X-ray</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/677/401/table14</name><description>Literature Class 0/I counterparts</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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