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<ri:Resource created="2023-03-21T14:36:30Z" 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>Correlations in unbound star trajectories</title><shortName>J/MNRAS/490/5647</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/490/5647</identifier><altIdentifier>doi:10.26093/cds/vizier.74905647</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Montanari F.</name></creator><creator><name>Barrado D.</name></creator><creator><name>Garcia-Bellido J.</name></creator><date role="Updated">2024-08-20T20:14:12Z</date><date role="Created">2023-03-21T14:36:30Z</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>high-velocity-stars</subject><subject>milky-way-galaxy</subject><subject>galaxies</subject><subject>globular-star-clusters</subject><subject>radial-velocity</subject><subject>proper-motions</subject><subject>stellar-distance</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>Scattering events with compact objects are expected in the primordial black hole (PBH) cold dark matter (CDM) scenario, due to close encounters between stars and PBHs in the dense environments of dwarf spheroidals. We develop a Bayesian framework to search for correlations among Milky Way stellar trajectories and those of globular clusters and dwarf galaxies in the halo and in other nearby galaxies. We apply the method to a selection of hypervelocity stars (HVS) and globular clusters from the Gaia DR2 catalogue and known nearby (mostly dwarf) galaxies with full phase-space and size measurements. We report positive evidence for trajectory intersection ~20-40Myr ago of up to two stars, depending on priors, with the Sagittarius dwarf spheroidal galaxy (dSph) when assuming the distance estimates of Marchetti, Rossi &amp; Brown (2019MNRAS.490..157M). We verify that the result is compatible with their evolutionary status, setting a lower bound for their stellar age of ~100Myr. However, such scattering events are not confirmed when assuming Anders et al. (2019A&amp;A...628A..94A, Cat. I/349) distance estimates. We discuss shortcomings related to present data quality and future prospects for detection of HVS with the full Gaia catalogue and Sagittarius dSph.</description><source format="bibcode">2019MNRAS.490.5647M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/490/5647</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Error on Dist</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Vx</name><description>? Galactocentric Cartesian velocity in X direction</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Vx</name><description>? Error on Vx</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vy</name><description>? Galactocentric Cartesian velocity in Y direction</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Vy</name><description>? Error on Vy</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Vz</name><description>? Galactocentric Cartesian velocity in Z direction</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Vz</name><description>? Error on Vz</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/490/5647/gc</name><description>Globular clusters</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">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>Name</name><description>Galaxy cluster name (NGCNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmRA</name><description>Proper motion in right ascension</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmDE</name><description>Proper motion in declination</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmRA</name><description>Error on pmRA</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_pmDE</name><description>Error on pmDE</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmRApmDEcor</name><description>Correlation between proper motion in right ascension and proper motion in declination</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV</name><description>Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>Error on RV</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>X position in cartesian heliocentric coordinates</description><unit>kpc</unit><ucd>pos.cartesian.x;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_X</name><description>Lower error on X</description><unit>kpc</unit><ucd>stat.error;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_X</name><description>Upper error on X</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>Y position in cartesian heliocentric coordinates</description><unit>kpc</unit><ucd>pos.cartesian.y;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Y</name><description>Lower error on Y</description><unit>kpc</unit><ucd>stat.error;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Y</name><description>Upper error on Y</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>Z position in cartesian heliocentric coordinates</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Z</name><description>Lower error on Z</description><unit>kpc</unit><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Z</name><description>Upper error on Z</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/490/5647/hvs</name><description>Hypervelocity stars</description><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>DE_ICRS</name><description>Declination (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>plx</name><description>Parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_plx</name><description>Error on plx</description><unit>mas</unit><ucd>stat.error;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmRA</name><description>Proper motion in right ascension</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</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>GaiaDR2</name><description>Gaia DR2 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>RA_ICRS</name><description>Right ascension (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>e_pmRA</name><description>Error on pmRA</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmDE</name><description>Proper motion in declination</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_pmDE</name><description>Error on pmDE</description><unit>mas/yr</unit><ucd>stat.error;pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>pmRApmDEcor</name><description>Correlation between proper motion in right ascension and proper motion in declination</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RV</name><description>Radial velocity derived in Marchetti et al. (2019MNRAS.490..157M)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_RV</name><description>Error on RV</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DistM</name><description>Distance derived in Marchetti et al. (2019MNRAS.490..157M)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_DistM</name><description>Lower error on DistM</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_DistM</name><description>Upper error on DistM</description><unit>pc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DistA</name><description>? Distance derived in Anders et al. (2019A&amp;A...628A..94A, Cat. I/349)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_DistA</name><description>? Lower error on DistA</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E_DistA</name><description>? Upper error on DistA</description><unit>pc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Pub</name><description>Probability of being unbound from the Milky Way potential (based on DistM)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>