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<ri:Resource created="2024-12-30T13:39:28Z" status="active" updated="2025-06-13T15:25:00Z" 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 LAMOST DR8</title><shortName>J/ApJ/942/109</shortName><identifier>ivo://CDS.VizieR/J/ApJ/942/109</identifier><altIdentifier>doi:10.26093/cds/vizier.19420109</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lei Z.</name></creator><creator><name>He R.</name></creator><creator><name>Nemeth P.</name></creator><creator><name>Vos J.</name></creator><creator><name>Zou X.</name></creator><creator><name>Hu Ke</name></creator><creator><name>Xiao H.</name></creator><creator><name>Yan H.</name></creator><creator><name>Zhao J.</name></creator><date role="Updated">2025-02-24T20:13:44Z</date><date role="Created">2024-12-30T13:39:28Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>effective-temperature</subject><subject>chemical-abundances</subject><subject>trigonometric-parallax</subject><description>A total of 222 hot subdwarf stars were identified with LAMOST DR8 spectra, among which 131 stars show composite spectra and have been decomposed, while 91 stars present single-lined spectra. Atmospheric parameters of all sample stars were obtained by fitting hydrogen (H) and helium (He) line profiles with synthetic spectra. Two long-period composite sdB binaries were newly discovered by combining our sample with the non-single-star data from Gaia DR3. One of the new systems presents the highest eccentricity (i.e., 0.5+/-0.09) among known wide sdB binaries, which is beyond model predictions. A total of 15 composite sdB stars fall in the high-probability binary region of the RUWE-AEN plane and deserve priority follow-up observations to further study their binary nature. A distinct gap is clearly presented among temperatures of cool companions for our composite-spectrum sample, but we could not come to a conclusion as to whether this feature is connected to the formation history of hot subdwarf stars before their binary natures are confirmed.</description><source format="bibcode">2023ApJ...942..109L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/942/109</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/VI/65">VI/65 : Evolutionary models of evolved stars (Dorman+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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