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<ri:Resource created="2011-11-21T13:20:11Z" 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>Spectroscopy of stars in the Galaxy's nuclear cluster</title><shortName>J/ApJ/703/1323</shortName><identifier>ivo://CDS.VizieR/J/ApJ/703/1323</identifier><altIdentifier>doi:10.26093/cds/vizier.17031323</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Do T.</name></creator><creator><name>Ghez A.M.</name></creator><creator><name>Morris M.R.</name></creator><creator><name>Lu J.R.</name></creator><creator><name>Matthews K.</name></creator><creator><name>Yelda S.</name></creator><creator><name>Larkin J.</name></creator><date role="Updated">2017-06-30T05:48:57Z</date><date role="Created">2011-11-21T13:20:11Z</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>line-intensities</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>early-type-stars</subject><subject>late-type-stars</subject><subject>milky-way-galaxy</subject><description>We report on the structure of the nuclear star cluster in the innermost 0.16pc of the Galaxy as measured by the number density profile of late-type giants. Using laser guide star adaptive optics in conjunction with the integral field spectrograph, OSIRIS, at the Keck II telescope, we are able to differentiate between the older, late-type (~1Gyr) stars, which are presumed to be dynamically relaxed, and the unrelaxed young (~6Myr) population. This distinction is crucial for testing models of stellar cusp formation in the vicinity of a black hole, as the models assume that the cusp stars are in dynamical equilibrium in the black hole potential. In the survey region, we classified 60 stars as early-type (O and early B; 22 newly identified) and 74 stars as late-type (K and M; 61 newly identified). We find that contamination from young stars is significant, with more than twice as many young stars as old stars in our sensitivity range (K'&lt;15.5) within the central arcsecond.</description><source format="bibcode">2009ApJ...703.1323D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/703/1323</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/A+A/534/A117">J/A+A/534/A117 : NIR polarimetry of sources near SgrA* (Buchholz+, 2011)</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/499/483">J/A+A/499/483 : NIR observations of sources in galactic center (Buchholz+,</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/ApJ/697/1741">J/ApJ/697/1741 : Warped disks of YSOs in Galactic center (Bartko+, 2009)</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/643/1011">J/ApJ/643/1011 : Early-type stars in the center of the Galaxy (Paumard+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/373/608">J/A+A/373/608 : Early-type stars towards the Galactic Center. 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