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<ri:Resource created="2025-06-04T09:51:29Z" status="active" updated="2026-07-02T12:01:15Z" 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>Binary fraction of young stars in ~0.4pc of the GC</title><shortName>J/ApJ/964/164</shortName><identifier>ivo://CDS.VizieR/J/ApJ/964/164</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-y4-54</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gautam A.K.</name></creator><creator><name>Do T.</name></creator><creator><name>Ghez A.M.</name></creator><creator><name>Chu D.S.</name></creator><creator><name>Hosek M.W.J.</name></creator><creator><name>Sakai S.</name></creator><creator><name>Naoz S.,Morris M.R.</name></creator><creator><name>Ciurlo A.</name></creator><creator><name>Haggard Z.</name></creator><creator><name>Lu J.R.</name></creator><date role="Updated">2026-07-02T12:01:15Z</date><date role="Created">2025-06-04T09:51:29Z</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>galactic-center</subject><subject>multiple-stars</subject><subject>eclipsing-binary-stars</subject><subject>infrared-photometry</subject><subject>stellar-ages</subject><subject>stellar-spectral-types</subject><subject>radial-velocity</subject><description>We present the first estimate of the intrinsic binary fraction of young stars across the central ~0.4pc surrounding the supermassive black hole (SMBH) at the Milky Way Galactic center (GC). This experiment searched for photometric variability in 102 spectroscopically confirmed young stars, using 119 nights of 10" wide adaptive optics imaging observations taken at W. M. Keck Observatory over 16yr in the K'-[2.1um] and H-[1.6um] bands. We photometrically detected three binary stars, all of which are situated more than 1" (0.04pc) from the SMBH and one of which, S2-36, is newly reported here with spectroscopic confirmation. All are contact binaries or have photometric variability originating from stellar irradiation. To convert the observed binary fraction into an estimate of the underlying binary fraction, we determined the experimental sensitivity through detailed light-curve simulations, incorporating photometric effects of eclipses, irradiation, and tidal distortion in binaries. The simulations assumed a population of young binaries, with stellar ages (4Myr) and masses matched to the most probable values measured for the GC young star population, and underlying binary system parameters (periods, mass ratios, and eccentricities) similar to those of local massive stars. As might be expected, our experimental sensitivity decreases for eclipses narrower in phase. The detections and simulations imply that the young, massive stars in the GC have a stellar binary fraction &gt;=71% (68% confidence), or &gt;=42% (95% confidence). This inferred GC young star binary fraction is consistent with that typically seen in young stellar populations in the solar neighborhood. Furthermore, our measured binary fraction is significantly higher than that recently reported by Chu et al. based on radial velocity measurements for stars &gt;~1" of the SMBH. Constrained with these two studies, the probability that the same underlying young star binary fraction extends across the entire region is &lt;1.4%. This tension provides support for a radial dependence of the binary star fraction, and therefore, for the dynamical predictions of binary merger and evaporation events close to the SMBH.</description><source format="bibcode">2024ApJ...964..164G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/964/164</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/ApJ/523/248">J/ApJ/523/248 : Variable stars in the Galactic center (Ott+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/597/323">J/ApJ/597/323 : Cool stars at the Galactic Center (Blum+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/154">J/ApJS/161/154 : Near-IR spectral atlas of OB stars (Hanson+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/643/1011">J/ApJ/643/1011 : Early-type stars in center of the Galaxy (Paumard+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/1241">J/ApJ/659/1241 : Stellar variability in Galactic Center (Rafelski+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/697/1741">J/ApJ/697/1741 : Warped disks of YSOs in Galactic center (Bartko+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/499/483">J/A+A/499/483 : NIR observations of sources in the GC (Buchholz+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/1323">J/ApJ/703/1323 : Spectroscopy of stars:Galaxy's nuclear cluster (Do+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/502/91">J/A+A/502/91 : Proper motions of stars near SgrA* (Schoedel+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A18">J/A+A/511/A18 : NIR observations of stars near SgrA* (Schoedel+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A146">J/A+A/537/A146 : Star models with rot. 0.8&lt;M&lt;120,Z=0.014 (Ekstrom+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/337.444">J/other/Sci/337.444 : RV curves of Galactic massive O stars (Sana+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/764/154">J/ApJ/764/154 : Stellar populations in the central 0.5pc. 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Mean Vega magnitude of star in H band (1)</description><unit>mag</unit><ucd>phot.mag;em.IR.H;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Age</name><description>Spectroscopically confirmed age of population (2)</description><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>n_Kpmag</name><description>[30/100] Number of K' band observations of star</description><ucd>meta.number;obs;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_Hmag</name><description>[0/19] Number of H band observations of star (1)</description><ucd>meta.number;obs;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>KprChi2</name><description>[0.1/274] Reduced {chi}^2^ from no variability model in K' band</description><ucd>stat.fit.chi2;meta.modelled;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HrChi2</name><description>[0.03/399]? Reduced {chi}^2^ from no variability model in H band (1)</description><ucd>stat.fit.chi2;meta.modelled;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KpVar</name><description>Variable in K' band? Yes/No</description><ucd>meta.code;src.var;em.IR.K</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>HVar</name><description>Variable in H band? Yes/No (1)</description><ucd>meta.code;src.var;em.IR.H</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Frac</name><description>[0.0/0.2] Fraction of injected binaries recovered from stellar light curve</description><ucd>stat;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>oRA</name><description>[-5.4/5.8] Offset East from Sgr A* position (17:45:40.0359 -29:00:28.169)</description><unit>arcsec</unit><ucd>pos.eq.ra;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>oDE</name><description>[-6.5/4.2] Offset North from Sgr A* position (17:45:40.0359 -29:00:28.169)</description><unit>arcsec</unit><ucd>pos.eq.dec;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>t0</name><description>Reference time for oRA, oDE in Julian years</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_RA</name><description>Position, computed from Sgr A* position (17:45:40.0359-29:00:28.169) with oRA and oDE offsets (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position, computed from Sgr A* position (17:45:40.0359-29:00:28.169) with oRA and oDE offsets (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/964/164/table1</name><description>Observations used in this experiment</description><column><name>Nbright</name><description>[185/490] Number of stars detected with mag_K'_&lt;=16</description><ucd>meta.number;src.sample;phot.mag</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nyoung</name><description>[55/99] Number of known young stars detected</description><ucd>meta.number;src.sample;time.age</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Date</name><description>UT Date</description><unit>'Y:M:D'</unit><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>f_Date</name><description>[n] Flag on UT date (1)</description><ucd>meta.code;time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MJD</name><description>Modified Julian Date of observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Filt</name><description>Bandpass (H or K')</description><ucd>instr.bandpass;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Ns</name><description>[186/1038] Number of sample stars detected</description><ucd>meta.number;src.sample</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MedErr</name><description>[0.02/0.12] Median photometric uncertainty of bright stars</description><unit>mag</unit><ucd>stat.error;phot.mag;stat.median</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/ApJ/964/164/table4</name><description>Photometric calibrator star bandpass corrected reference fluxes</description><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Name</name><description>Name of star</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SpType</name><description>Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>KsS10</name><description>[10.1/15.0] Ks band Vega magnitude from S10 (1)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_KsS10</name><description>[0.06/0.09] Uncertainty in Ks_S10_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dKmag</name><description>[-0.07/-0.04] Magnitude difference, Ks_S10_-K'_NIRC2_</description><unit>mag</unit><ucd>phot.mag;arith.diff;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dKmag</name><description>[0.01]? Uncertainty in dKmag</description><unit>mag</unit><ucd>stat.error;phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>KpNIRC2</name><description>[10.1/15.1] K' band NIRC2 Vega magnitude, this article</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_KpNIRC2</name><description>[0.06/0.09] Uncertainty in K'_NIRC2_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HS10</name><description>[12.0/16.9] H band Vega magnitude from S10 (1)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HS10</name><description>[0.06/0.09] Uncertainty in H_S10_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dHmag</name><description>[-0.20/-0.13] Magnitude difference, H_S10_-H_NIRC2_</description><unit>mag</unit><ucd>phot.mag;arith.diff;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_dHmag</name><description>[0.01]? Uncertainty in dHmag</description><unit>mag</unit><ucd>stat.error;phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HNIRC2</name><description>[12.1/16.7] H band NIRC2 Vega magnitude, this article</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HNIRC2</name><description>[0.07/0.10] Uncertainty in H_NIRC2_</description><unit>mag</unit><ucd>stat.error;phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S10</name><description>Display data from Schoedel+ 2010, J/A+A/511/A18 within 0.08"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>