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<ri:Resource created="2011-06-21T10:08:25Z" 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>The Chandra survey of the SMC "Bar". II.</title><shortName>J/ApJ/697/1695</shortName><identifier>ivo://CDS.VizieR/J/ApJ/697/1695</identifier><altIdentifier>doi:10.26093/cds/vizier.16971695</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Antoniou V.</name></creator><creator><name>Zezas A.</name></creator><creator><name>Hatzidimitriou D.</name></creator><creator><name>McDowell J.C.</name></creator><date role="Updated">2017-10-09T13:33:35Z</date><date role="Created">2011-06-21T10:08:25Z</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>magellanic-clouds</subject><subject>x-ray-binary-stars</subject><subject>be-stars</subject><description>We present the most likely optical counterparts of 113 X-ray sources detected in our Chandra survey of the central region of the Small Magellanic Cloud (SMC) based on the OGLE-II and Magellanic Clouds Photometric Survey catalogs. We estimate that the foreground contamination and chance coincidence probability are minimal for the bright optical counterparts (corresponding to OB type stars; 35 in total). We propose here for the first time 13 high-mass X-ray binaries, of which four are Be/X-ray binaries (Be-XRBs), and we confirm the previous classification of 18 Be-XRBs. We estimate that the new candidate Be-XRBs have an age of ~15-85Myr, consistent with the age of Be stars.</description><source format="bibcode">2009ApJ...697.1695A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/697/1695</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/I/315">I/315 : UCAC3 Catalogue (Zacharias+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/denis">B/denis : The DENIS database (DENIS Consortium, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/234">VII/234 : DENIS catalog of galaxies (Paturel+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/284">I/284 : The USNO-B1.0 Catalog (Monet+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/236">II/236 : UBVR CCD survey of the Magellanic clouds (Massey+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/271">I/271 : The Guide Star Catalog, Version 2.2 (GSC2.2) (STScI, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/228">II/228 : DENIS Catalogue toward Magellanic Clouds (DCMC) (Cioni+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/221">I/221 : The Magellanic Catalogue of Stars - MACS (Tucholke+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/388/1198">J/MNRAS/388/1198 : Be/X-ray binaries in Small Magellanic Cloud (McBride+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/54/1">J/AcA/54/1 : OGLE II SMC eclipsing binaries (Wyrzykowski+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/353/705">J/MNRAS/353/705 : OGLE Variables in Magellanic Clouds (Ita+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1632">J/AJ/127/1632 : UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/353/601">J/MNRAS/353/601 : 2dF survey of the Small Magellanic Cloud (Evans+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/161">J/PASJ/55/161 : ASCA sources in the SMC (Yokogawa+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/48/147">J/AcA/48/147 : OGLE SMC BVI photometry (Udalski+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/48/563">J/AcA/48/563 : Photometry of OGLE SMC eclipsing binaries (Udalski+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/51/317">J/AcA/51/317 : OGLE DIA. 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Degree of Declination of optical source</description><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column></table><table><name>J/ApJ/697/1695/table4</name><description>Additional optical info</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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