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<ri:Resource created="2011-10-25T14:23:38Z" 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>HST/NICMOS III imaging in Orion Nebula Cluster</title><shortName>J/A+A/534/A10</shortName><identifier>ivo://CDS.VizieR/J/A+A/534/A10</identifier><altIdentifier>doi:10.26093/cds/vizier.35340010</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andersen M.</name></creator><creator><name>Meyer M.R.</name></creator><creator><name>Robberto M.</name></creator><creator><name>Bergeron L.E.</name></creator><creator><name>Reid N.</name></creator><date role="Updated">2011-12-27T15:02:58Z</date><date role="Created">2011-10-25T14:23:38Z</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>pre-main-sequence-stars</subject><subject>hst-photometry</subject><description>We present deep HST/NICMOS Camera 3 F110W and F160W imaging of a 26'x33', corresponding to 3.1x3.8pc^2^, non-contiguous field towards the Orion Nebula Cluster (ONC). The main aim is to determine the ratio of low-mass stars to brown dwarfs for the cluster as a function of radius out to a radial distance of 1.5pc. The sensitivity of the data outside the nebulous central region is F160W&lt;=21.0mag, significantly deeper than previous studies of the region over a comparable area. We create an extinction limited sample and determine the ratio of low-mass stars (0.08-1M_{sun}_) to brown dwarfs (0.02-0.08M_{sun}_ and 0.03-0.08M_{sun}_) for the cluster as a whole and for several annuli. The ratio found for the cluster within a radius of 1.5pc is R_02_=N(0.08-1M_{sun}_)/N(0.02-0.08M_{sun}_)=1.7+/-0.2, and R_03_=N(0.08-1M_{sun}_)/N(0.03-0.08M_{sun}_)=2.4+/-0.2, after correcting for field stars. The ratio for the central 0.3x0.3pc^2^ region down to 0.03M_{sun}_ was previously found to be R_03_=3.3^+0.8^_-0.7_, suggesting the low-mass content of the cluster is mass segregated. We discuss the implications of a gradient in the ratio of stars to brown dwarfs in the ONC in the context of previous measurements of the cluster and for other nearby star forming regions. We further discuss the current evidence for variations in the low-mass IMF and primordial mass segregation.</description><source format="bibcode">2011A&amp;A...534A..10A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/534/A10</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/AJ/120/1426">J/AJ/120/1426 : Chandra sources in ONC + BN-KL (Garmire+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/1676">J/AJ/121/1676 : ONC low-mass stars photometry (Rebull+, 2001)</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><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/1462">J/ApJ/660/1462 : Abundances of ONC X-ray PMS stars (Maggio+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/605">J/ApJ/671/605 : NGC 2264 and ONC PMS stars in the infrared (Cieza+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/677/401">J/ApJ/677/401 : X-ray properties of protostars in ONC (Prisinzano+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/261">J/ApJS/183/261 : Optical photometry of the ONC (Da Rio+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/400/603">J/MNRAS/400/603 : New variables in ONC (Parihar+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/502/883">J/A+A/502/883 : ONC very low mass stars I phot. 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