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<ri:Resource created="2020-03-05T08:16:13Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Crosscorrelation function (CCF) studies in GX 17+2</title><shortName>J/ApJS/244/5</shortName><identifier>ivo://CDS.VizieR/J/ApJS/244/5</identifier><altIdentifier>doi:10.26093/cds/vizier.22440005</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sriram K.</name></creator><creator><name>Malu S.</name></creator><creator><name>Choi C.S.</name></creator><date role="Updated">2020-04-30T07:57:57Z</date><date role="Created">2020-03-05T08:16:13Z</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>x-ray-binary-stars</subject><subject>x-ray-sources</subject><description>Neutron star Z-type sources provide a unique platform in order to understand the structure of accretion disk-corona geometry emitting close to the Eddington luminosity. Using RXTE and Nuclear Spectroscopic Telescope Array Mission (NuSTAR) satellite data, we performed crosscorrelation function (CCF) studies in GX 17+2 in order to constrain the size of the corona responsible for hard X-rays. From the RXTE data, we found that during horizontal and normal branches, the CCFs show anticorrelated hard (16-30keV) and soft (2-5keV) X-ray delays of the order of a few tens to hundred seconds with a mean correlation coefficient of 0.42+/-0.11. Few observations shows correlated lags and, on one occasion, coincident with radio emission. We also report an anticorrelated hard X-ray delay of 113+/-51s using the NuSTAR data of GX 17+2. Based on RXTE data, we find that soft and hard X-ray fluxes are varying, indicating the changes in the disk-corona structure during delays. We bridle the size of the corona using relativistic precession, transition layer models, and boundary layer models. Assuming the delays to be a readjustment timescale of the disk-corona structure, the height of the corona was estimated to be ~17-100km. Assuming that the inner region of the truncated disk is occupied by the corona, we constrain the coronal readjustment velocities (v_corona_={beta}v_disk_, where v_disk_ is the radial velocity component of the disk) of the order of {beta}=0.06-0.12. This study indicates that the observed delays are primarily dependent on the varying coronal readjustment velocities.</description><source format="bibcode">2019ApJS..244....5S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/244/5</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/cb">B/cb : Cataclysmic Binaries, LMXBs, and related objects (Ritter+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/106">V/106 : Catalogue of X-ray binaries (Liu+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/281/161">J/A+A/281/161 : Radio emission from stars at 250GHz (Altenhoff+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/411/L59">J/A+A/411/L59 : INTEGRAL reference catalog (Ebisawa+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/458/21">J/A+A/458/21 : INTEGRAL burst observations of 4U 1728-34 (Falanga+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/179/360">J/ApJS/179/360 : Thermonuclear X-ray bursts observed by RXTE (Galloway+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/1">J/ApJS/186/1 : The 4th IBIS/ISGRI soft gamma-ray survey catalog (Bird+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/522/A68">J/A+A/522/A68 : Variable sources detected by INTEGRAL (Telezhinsky+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/129">J/AJ/141/129 : Chandra Transmission Grating Data Cat. 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Lag</description><unit>s</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></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>ObsID</name><description>Observation identifier</description><ucd>meta.id;obs.param;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Sec</name><description>Light curve section identifier</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Start</name><description>Observation Start, UT date</description><unit>s</unit><ucd>time.start;obs</ucd><flag>nullable</flag></column><column><name>End</name><description>Observation Stop, UT date</description><unit>s</unit><ucd>time.end;obs</ucd><flag>nullable</flag></column><column><name>Texp</name><description>[533/42117] Total exposure time</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CC</name><description>[-0.8/1]? Cross-correlation coefficient</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_CC</name><description>[0.008/0.3]? Uncertainty in CC</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HR1</name><description>[0.01/0.06] Hardness Ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HR2</name><description>[0.01/0.09] Hardness Ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HID</name><description>Position in the hardness intensity diagram (HID)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>B_Lag</name><description>[-766/1364]? Upper bound on Lag</description><unit>s</unit><ucd>time.interval;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>b_Lag</name><description>[-636/1638]? Lower bound on Lag</description><unit>s</unit><ucd>time.interval;stat.min</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>