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<ri:Resource created="2010-03-10T17:18:14Z" 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>Canis Major R1 X-ray sources</title><shortName>J/A+A/506/711</shortName><identifier>ivo://CDS.VizieR/J/A+A/506/711</identifier><altIdentifier>doi:10.26093/cds/vizier.35060711</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gregorio-Hetem J.</name></creator><creator><name>Montmerle T.</name></creator><creator><name>Rodrigues C.V.</name></creator><creator><name>Marciotto E.,Preibisch T.</name></creator><creator><name>Zinnecker H.</name></creator><date role="Updated">2010-03-10T16:26:36Z</date><date role="Created">2010-03-10T17:18:14Z</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>stellar-associations</subject><subject>x-ray-sources</subject><subject>pre-main-sequence-stars</subject><subject>infrared-photometry</subject><description>The CMa R1 star-forming region contains several compact clusters as well as many young early-B stars. It is associated with a well-known bright rimmed nebula, the nature of which is unclear (fossil HII region or supernova remnant). To help elucidate the nature of the nebula, our goal was to reconstruct the star-formation history of the CMa R1 region, including the previously unknown older, fainter low-mass stellar population, using X-rays. We analyzed images obtained with the ROSAT satellite, covering ~5deg^2^. Complementary VRI photometry was performed with the Gemini South telescope. 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