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<ri:Resource created="2021-12-13T09:52:56Z" 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>Hot subdwarf stars from Gaia with LAMOST sp. II. RVs</title><shortName>J/ApJ/898/64</shortName><identifier>ivo://CDS.VizieR/J/ApJ/898/64</identifier><altIdentifier>doi:10.26093/cds/vizier.18980064</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luo Y.</name></creator><creator><name>Nemeth P.</name></creator><creator><name>Li Q.</name></creator><date role="Updated">2022-10-04T11:56:06Z</date><date role="Created">2021-12-13T09:52:56Z</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>subdwarf-stars</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><description>Combining LAMOST radial velocities with Gaia parallaxes and proper motions, we present 3D Galactic space motions and the orbits of 182 single-lined hot subdwarf stars. These stars were identified by Lei+ (Paper I; 2020, J/ApJ/889/117) in Gaia DR2 with LAMOST DR6 and DR7 spectra. He-rich hot subdwarf stars with log(y)&gt;=0 show the largest standard deviations of the Galactic velocity components and orbital parameters, while those with -1&lt;=log(y)&lt;=0 exhibit the second largest standard deviations. The two groups of He-deficient stars with log(y){&lt;}-1 show similar standard deviations, which are systematically lower compared to He-rich stars. We also present a kinematic population classification of the four hot subdwarf helium groups based on their positions in the U-V velocity diagram, the J_Z_- eccentricity diagram, and their Galactic orbits. The overall tendency of the fractional distributions of the four hot subdwarf helium groups in the halo, thin disk, and thick disk is largely consistent with the findings reported by Luo+ (2019ApJ...881....7L) based on LAMOST DR5, which appears to support predictions of binary population synthesis. He-deficient stars with -2.2&lt;=log(y){&lt;}-1 likely originate from a stable Roche lobe overflow channel, He-deficient stars with log(y){&lt;}-2.2 from the common envelope ejection channel, and He-rich stars with log(y)&gt;=0 from the merger channel of double He white dwarf stars. The fraction of He-rich hot subdwarf stars with -1&lt;=log(y)&lt;0 in the thin disk and the halo is far higher than that in the thick disk, which implies that these stars have different formation channels in the thin disk and in the halo.</description><source format="bibcode">2020ApJ...898...64L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/898/64</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/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/164">V/164 : LAMOST DR5 catalogs (Luo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/400/939">J/A+A/400/939 : Stellar parameters of 115 HQS sdB stars (Edelmann+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/400/877">J/A+A/400/877 : White dwarfs 3D kinematics from SPY project (Pauli+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/223">J/A+A/430/223 : Parameters of cool companions of sdB stars (Lisker+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/447/173">J/A+A/447/173 : 3D-kinematics of WDs from SPY project. 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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>e_zmax</name><description>[0.01/472] Standard error in zmax</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RA_ICRS</name><description>Barycentric Right Ascension (ICRS) at Epoch=2000.0</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DE_ICRS</name><description>[-3.1/82] Barycentric Declination (ICRS) at Epoch=2000.0</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Teff</name><description>[22230/79240] Stellar effective temperature (2)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>[10/11150] Standard error in Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[5/6.9] Stellar surface gravity (2)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>[0/0.8] Standard error in logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(y)</name><description>[-3.5/2.81] Stellar surface He abundance y=n(He)/n(H) (2)</description><unit>log(Sun)</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(y)</name><description>[0.01/1.04]? 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xsi:type="vs:VOTableType">float</dataType></column><column><name>dist</name><description>[279/8850] Gaia DR2 stellar distance</description><unit>pc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SpT</name><description>Spectral type (2)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>e_dist</name><description>[6/8427] Standard error in dist</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RVel</name><description>[-352/206] Radial velocity from LAMOST spectra</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_RVel</name><description>[12/78] Standard error in RVelal velocity</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType 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xsi:type="vs:VOTableType">float</dataType></column><column><name>Rperi</name><description>[0.06/14.3] Pericenter radius (3)</description><unit>kpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Rperi</name><description>[0.01/8.5] Standard error in Rperi</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zmax</name><description>[0.09/372] Maximum vertical height (3)</description><unit>kpc</unit><ucd>pos.cartesian.z;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_e</name><description>[0.01/0.22] Standard error in e</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Jz</name><description>[-3515/2972] Z-component of angular momentum (3)</description><unit>kpc.km**-1.s**-1</unit><ucd>phys.angMomentum</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Jz</name><description>[8.3/2962] Standard error in Jz</description><unit>kpc.km**-1.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zn</name><description>[0.01/8.5] Normalised z-extent of the orbit (3)</description><ucd>src.orbital</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zn</name><description>[0/38.5] Standard error in zn</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pop</name><description>Population classification (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>p(TH)</name><description>[0/95] Probability in thin disk</description><unit>%</unit><ucd>stat</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>p(TK)</name><description>[0/99] Probability in 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