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<ri:Resource created="2023-04-13T09:02:27Z" 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>Gaia stellar flyby analysis for spiral arm hosts</title><shortName>J/ApJS/263/31</shortName><identifier>ivo://CDS.VizieR/J/ApJS/263/31</identifier><altIdentifier>doi:10.26093/cds/vizier.22630031</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shuai L.</name></creator><creator><name>Ren B.B.</name></creator><creator><name>Dong R.</name></creator><creator><name>Zhou X.</name></creator><creator><name>Pueyo L.</name></creator><creator><name>De Rosa R.J.</name></creator><creator><name>Fang T.,Mawet D.</name></creator><date role="Updated">2023-08-25T11:33:11Z</date><date role="Created">2023-04-13T09:02:27Z</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>stellar-radii</subject><subject>stellar-distance</subject><subject>young-stellar-objects</subject><subject>infrared-sources</subject><subject>visible-astronomy</subject><subject>surveys</subject><description>Scattered-light imaging studies have detected nearly two dozen spiral arm systems in circumstellar disks, yet the formation mechanisms for most of them are still under debate. Although existing studies can use motion measurements to distinguish leading mechanisms such as planet-disk interaction and disk self-gravity, close-in stellar flybys can induce short-lived spirals and even excite arm-driving planets into highly eccentric orbits. With unprecedented stellar location and proper-motion measurements from Gaia Data Release 3 (DR3), here we study for known spiral arm systems their flyby history with their stellar neighbors by formulating an analytical on-sky flyby framework. For stellar neighbors currently located within 10pc of the spiral hosts, we restrict the flyby time to within the past 10^4^yr and the flyby distance to within 10 times the disk extent in scattered light. Among a total of 12570 neighbors that are identified in Gaia DR3 for 20 spiral systems, we do not identify credible flyby candidates for isolated systems. Our analysis suggests that a close-in recent flyby is not the dominant formation mechanism for isolated spiral systems in scattered light.</description><source format="bibcode">2022ApJS..263...31S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/263/31</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/eso">B/eso : ESO Science Archive Catalog (ESO, 1991-2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/458/173">J/A+A/458/173 : Optical spectroscopy of 253 IRAS sources (Suarez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/1964">J/ApJ/703/1964 : Spectra of three nearby star-forming regions (Furlan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/121">J/ApJ/783/121 : BANYAN II. Nearby young assoc. cand. members (Gagne+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/786/97">J/ApJ/786/97 : Photospheric properties of T Tauri stars (Herczeg+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/188">J/AJ/153/188 : Spectroscopy of the foreground pop. in Orion A (Fang+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/95">J/AJ/153/95 : Catalog of Suspected Nearby Young Stars (Riedel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/23">J/ApJ/856/23 : BANYAN. XI. The BANYAN {Sigma} algorithm (Gagne+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/898/L38">J/ApJ/898/L38 : VLT/SPHERE Y-band images of MWC 758 at two epochs (Ren+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/163/219">J/AJ/163/219 : Gaia DR2 stellar flybys in the Sco-Cen OB assoc. (Ma+, 2022)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/263/31</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/263/31</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/263/31</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/263/31</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/263/31</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Host</name><description>Spiral host name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType><flag>primary</flag></column><column><name>Rdisk</name><description>[17/438] Approximate disk radius in scattered light matching field of view in Figure 1</description><unit>AU</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nn</name><description>Number of neighboring stars (link to Table 2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Nbr</name><description>[201/1973] Number of neighboring stars in Gaia DR3 with location and proper-motion measurements within 10pc</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nf</name><description>[2/28] Number of neighboring stars whose closest approach to the host is within 10^4^yr before Gaia DR3</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dca</name><description>[203/945081] Expectation for closest on-sky approach distance in the frequentist approach (1)</description><unit>AU</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Dca</name><description>[0/2892] Standard deviation in Dca</description><unit>AU</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>zScore</name><description>[1.5/14326] Minimum z-score for the closest approaches of all neighbors (1) (2)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RUWE</name><description>[0.9/3.7] RUWE of the host star in Gaia DR3</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></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>f_RUWE</name><description>[b] Flag on RUWE (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><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></table><table><name>J/ApJS/263/31/table2</name><description>Flyby history of the 20 source neighbors using Gaia DR3</description><column><name>Host</name><description>Stellar identifier</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2016. (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</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>Gaia</name><description>Gaia DR3 unique source designation</description><ucd>meta.id;meta.main</ucd></column><column><name>Dca</name><description>[0/11021317] Closest approach distance (1)</description><unit>AU</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Dca</name><description>[0/24144] Standard deviation in Dclose</description><unit>AU</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tca</name><description>[-10000/0] Closest approach time (1)</description><unit>AU</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zScore</name><description>[1.5/2882927057]? The z-score (Dca/e_Dca)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RA_ICRS</name><description>[54.4/257.1] Right Ascension (ICRS) at Ep=2016.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>[-84.4/34.2] Declination (ICRS) at Ep=2016.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>RUWE</name><description>[0.6/49] Gaia DR3 Renormalised Unit Weight Error for each source</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>