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<ri:Resource created="2014-04-09T12:25:50Z" 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>Mass accretion rates from HST in the ONC</title><shortName>J/ApJ/755/154</shortName><identifier>ivo://CDS.VizieR/J/ApJ/755/154</identifier><altIdentifier>doi:10.26093/cds/vizier.17550154</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Manara C.F.</name></creator><creator><name>Robberto M.</name></creator><creator><name>Da Rio N.</name></creator><creator><name>Lodato G.</name></creator><creator><name>Hillenbrand L.A.,Stassun K.G.</name></creator><creator><name>Soderblom D.R.</name></creator><date role="Updated">2017-06-12T08:25:05Z</date><date role="Created">2014-04-09T12:25:50Z</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>accretion</subject><subject>open-star-clusters</subject><subject>hst-photometry</subject><subject>line-intensities</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><description>The present observational understanding of the evolution of the mass accretion rates (dM/dt_acc_) in pre-main-sequence stars is limited by the lack of accurate measurements of dM/dt_acc_ over homogeneous and large statistical samples of young stars. Such observational effort is needed to properly constrain the theory of star formation and disk evolution. Based on Hubble Space Telescope/WFPC2 observations, we present a study of dM/dt_acc_ for a sample of ~700 sources in the Orion Nebula Cluster, ranging from the hydrogen-burning limit to M*~2M_{sun}_. We derive dM/dt_acc_ from both the U-band excess and the H{alpha} luminosity (L_H{alpha}_), after determining empirically both the shape of the typical accretion spectrum across the Balmer jump and the relation between the accretion luminosity (L_acc_) and L_H{alpha}_, which is L_acc_/L_{sun}_=(1.31+/-0.03).L_H{alpha}/L_{sun}_+(2.63+/-0.13). Given our large statistical sample, we are able to accurately investigate relations between dM/dt_acc_ and the parameters of the central star such as mass and age.</description><source format="bibcode">2012ApJ...755..154M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/755/154</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/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/28">J/ApJS/208/28 : H{alpha} survey in the ONC (Szegedi-Elek+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/10">J/ApJS/207/10 : HST Treasury Program on the ONC (Robberto+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/14">J/ApJ/748/14 : ONC population data from WFI observations (Da Rio+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/1092">J/ApJ/722/1092 : Optical photometry of the ONC. II. (Da Rio+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A10">J/A+A/534/A10 : HST/NICMOS III imaging in ONC (Andersen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2136">J/AJ/136/2136 : HST/ACS Atlas of Great Orion Nebula proplyds (Ricci+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/374/1413">J/MNRAS/374/1413 : SCUBA survey of Orion (Nutter+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/642/1140">J/ApJ/642/1140 : Disk mass loss in the Orion Nebula Cluster (Olczak+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/363">J/AJ/129/363 : Spectroscopy in Orion Nebula Cluster (Sicilia-Aguilar+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/111/846">J/AJ/111/846 : Orion HST survey (O'Dell+ 1996)</relatedResource><relatedResource>http://archive.stsci.edu/prepds/orion/ : HST Treasury Program on the ONC</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/755/154</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/755/154</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/755/154</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/755/154</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/755/154</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/755/154</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/755/154/2cd (Stellar parameters and accretion values of the sources with A_V_ and L_acc_ determined from the 2CD method)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/755/154/2cd?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/755/154/2cd?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/755/154/2cd?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>83.5628625</ra><dec>-5.383325278</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/755/154/dario (Stellar parameters and accretion values of the sources with A_V_ from Da Rio+ (Cat. 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