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<ri:Resource created="2020-12-21T15:37:51Z" 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>Vertical motions of APOGEE &amp; Gaia red clump stars</title><shortName>J/ApJ/878/21</shortName><identifier>ivo://CDS.VizieR/J/ApJ/878/21</identifier><altIdentifier>doi:10.26093/cds/vizier.18780021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ting Y.-S.</name></creator><creator><name>Rix H.-W.</name></creator><date role="Updated">2023-06-08T08:34:55Z</date><date role="Created">2020-12-21T15:37:51Z</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>chemical-abundances</subject><subject>stellar-ages</subject><subject>stellar-distance</subject><description>It has long been known that the vertical motions of Galactic disk stars increase with stellar age, commonly interpreted as vertical heating through orbit scattering. Here we map the vertical actions of disk stars as a function of age ({tau}&lt;=8Gyr) and across a large range of Galactocentric radii, R_GC_, drawing on APOGEE and Gaia data. We fit J_z_(R_GC,{tau}_) as a combination of the vertical action at birth, J_z,0_, and the subsequent heating {Delta}J_z,1Gyr_(R_GC_), which scales as {tau}^{gamma}(R_GC_)^. The inferred birth temperature, J_z,0_(R_GC_) is 1kpc.km/s for 3kpc&lt;R_GC_&lt;10kpc, consistent with the ISM velocity dispersion, but it rapidly rises outward, to 8kpc.km/s for R_GC_=14kpc, likely reflecting the stars' birth in a warped or flared gas disk. We find the heating rate {Delta}J_z,1Gyr_ to be modest and nearly constant across all radii, 1.6kpc.km/s/Gyr. The stellar age dependence {gamma} gently grows with Galactocentric radius, from {gamma}~1 for R_GC_&lt;~R_{sun}_ to {gamma}~1.3 at R_GC_=14kpc. The observed J_z_-{tau} relation at all radii is considerably steeper ({gamma}&gt;~1) than the time dependence theoretically expected from orbit scattering, J_z_{propto}t^0.5^. We illustrate how this conundrum can be resolved if we also account for the fact that at earlier epochs, the scatterers were more common, and the restoring force from the stellar disk surface mass density was low. Our analysis may reinstate gradual orbital scattering as a plausible and viable mechanism to explain the age-dependent vertical motions of disk stars.</description><source format="bibcode">2019ApJ...878...21T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/878/21</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/V/117">V/117 : Geneva-Copenhagen Survey of Solar neighbourhood (Holmberg+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/130">V/130 : Geneva-Copenhagen Survey of Solar neighbourhood III (Holmberg+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/284">III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/480/91">J/A+A/480/91 : Gal. disk stars vertical distribution. 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Red clump stars selected from LAMOST and APOGEE (Ting+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/32">J/ApJS/239/32 : APOKASC-2 cat. of Kepler evolved stars (Pinsonneault+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/872/95">J/ApJ/872/95 : GALEX &amp; Gaia data for APOGEE red clump stars (Mohammed+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/872/137">J/ApJ/872/137 : Abund. of red clump &amp; RGB stars with APOGEE (Shetrone+, 2019)</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/ApJ/878/21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/878/21</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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29890-29892 29894 29896-29897 29900 29912 29916 29918 29920 29922-29923 29928-29930 29940 29997 30029 30034 30042 30064-30065 30141 30143 30184 30186 30190 30212-30213 30215-30216 30218-30220 30222-30224 30226-30227 30233 30240-30241 30244 30246-30247 30254 30260 30262-30265 30268-30269 30274 30280 30292-30293 30295 30301-30302 30307 30310 30321 30323 30328 30331-30332 30336-30338 30340 30342-30343 30349 30358 30364 30380-30381 30383-30384 30386-30387 30389 30392-30393 30401 30404-30405 30415-30417 30419-30422 30426-30427 30441 30452 30454 30456-30457 30464 30466 30472-30474 30485 30496 30498 30524-30525 30527-30529 30532-30533 30544-30546 30550 30552-30553 30556 30560 30562 30568 30570 30618-30619 30621-30623 30641 30644-30646 30667 30670 30675 30678-30679 30681 30689 30691 30697 30700-30701 30707 30710-30711 30747 30770-30772 30774 30776 30780 30831 30857 30862 30973 31056 31060 31138 31144 31147 31378 31601 31604 31748 31750-31751 31753 31756-31757 31768 31797 31818 32005 32007 32013 32016 32018-32019 32023-32026 32029 32043 32053 32071 32073-32075 32077 32079 32082 32092 32097 32102 32112-32113 32129 32132-32134 32145 32147-32148 32150-32151 32156 32460 32466 32497 32500 32502 32509 32701 32703 32754 36689 36727 36739-36740 36856 39915 39918 39933 39935 40622 40625 40627 40633 40666-40667 40670 40674 40677 40679-40680 40694 40739 40742 40744-40746 40748-40750 40798 40819-40821 40897 44771 47871 48033 48035 48056 48925</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/878/21?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/878/21/table1</name><description>APOGEE red clump value-added catalog</description><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>APOGEE</name><description>APOGEE identifier (from Ting+, 2018, J/ApJ/858/L7)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>[Fe/H]</name><description>[-0.7/0.4] Abundance, [Fe/H] (1)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Mg/Fe]</name><description>[-0.15/0.3] Abundance, [Mg/Fe] (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gaia</name><description>Gaia DR2 (I/345) source identifier</description><ucd>meta.id.cross</ucd></column><column><name>RA_ICRS</name><description>Gaia DR2 Right Ascension (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DE_ICRS</name><description>Gaia DR2 Declination (ICRS) at Ep=2015.5</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>Age</name><description>[0.16/8] Stellar age (2)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Dist</name><description>[0.026/8.8] Inferred photometric red clump distance from the Sun</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Rgc</name><description>[3/16.4] Galactocentric observed radius</description><unit>kpc</unit><ucd>phys.size.radius;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Zgc</name><description>[-0.5/0.5] Galactic observed height</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RgcBirth</name><description>[0.00095/17.4]? Inferred birth radius</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RgcMean</name><description>[1.8/14.7]? Mean Radius (3)</description><unit>kpc</unit><ucd>phys.size.radius;stat.mean</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>JR</name><description>[0/1492]? Radial phase space action</description><unit>kpc.km/s</unit><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Lz</name><description>[-125/6580] Angular momentum phase space action</description><unit>kpc.km/s</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Jz</name><description>[9e-5/1000] Vertical phase space action</description><unit>kpc.km/s</unit><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DR16</name><description>Display data from APOGEE-2 DR16 catalog (III/284)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</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>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2015.5 (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=J2015.5 (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></table></schema></tableset></ri:Resource>