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<ri:Resource created="2020-12-02T09:55:52Z" 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>Chandra X-ray sources in the globular cluster 47 Tuc</title><shortName>J/ApJ/876/59</shortName><identifier>ivo://CDS.VizieR/J/ApJ/876/59</identifier><altIdentifier>doi:10.26093/cds/vizier.18760059</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cheng Z.</name></creator><creator><name>Li Z.</name></creator><creator><name>Li X.</name></creator><creator><name>Xu X.</name></creator><creator><name>Fang T.</name></creator><date role="Updated">2021-09-09T09:43:26Z</date><date role="Created">2020-12-02T09:55:52Z</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>globular-star-clusters</subject><subject>x-ray-sources</subject><description>Using archival Chandra observations with a total exposure of 510ks, we present an updated catalog of point sources for globular cluster (GC) 47 Tucanae. Our study covers an area of ~176.7'^2^ (i.e., with R&lt;~7.5') with 537 X-ray sources. We show that the surface density distribution of X-ray sources in 47 Tuc is highly peaked in the cluster center, rapidly decreases at intermediate radii, and finally rises again at larger radii, with two distribution dips at R~100" and R~170" for the faint (L_X_&gt;~5.0x10^30^erg/s) and bright (L_X_&lt;~5.0x10^30^erg/s) groups of X-ray sources, respectively. These distribution features are similar to those of blue straggler stars (BSSs), where the distribution dip is located at R~200". By fitting the radial distribution of each group of sources with a "generalized King model", we estimated an average mass of 1.51+/-0.17M_{sun}_, 1.44+/-0.15M_{sun}_ and 1.16+/-0.06M_{sun}_ for the BSSs, bright X-ray sources, and faint X-ray sources, respectively. These results are consistent with the mass segregation effect of heavy objects in GCs, where more massive objects drop to the cluster center faster and their distribution dip propagates outward further. Besides, the peculiar distribution profiles of X-ray sources and BSSs are also consistent with the mass segregation model of binaries in GCs, which suggests that, in addition to the dynamical formation channel, primordial binaries are also a significant contributor to the X-ray source population in GCs.</description><source format="bibcode">2019ApJ...876...59C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/876/59</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/chandra">B/chandra : The Chandra Archive Log (CXC, 1999-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/150">V/150 : Updated cat. of variable stars in globular clusters (Clement+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/113/299">J/A+AS/113/299 : Abundances &amp; vel. for cluster giants (Minniti 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/109/218">J/AJ/109/218 : Catalogue of globular cluster profiles (Trager+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/324/915">J/A+A/324/915 : Blue stragglers in M3 (Ferraro+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/559/1060">J/ApJ/559/1060 : Variables in 47 Tuc (Albrow+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/292.2290">J/other/Sci/292.2290 : Chandra compact binaries in 47 Tuc (Grindlay+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/391/945">J/A+A/391/945 : HST phot. of 74 gal. globular clusters (Piotto+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/632/894">J/ApJ/632/894 : Blue stragglers, HB &amp; turnoff stars (De Marco+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/625/796">J/ApJ/625/796 : X-ray sources in the 47 Tuc GCs (Heinke+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/166/249">J/ApJS/166/249 : Stellar dynamics and PMs in 47Tuc (McLaughlin+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/447">J/AJ/132/447 : Surface Brightness of 38 Gal. 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