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<ri:Resource created="2024-02-23T07:04:17Z" 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>OB-stars observed at 1450MHz</title><shortName>J/AJ/166/23</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/23</identifier><altIdentifier>doi:10.26093/cds/vizier.51660023</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Huang Q.</name></creator><creator><name>Jiang B.</name></creator><creator><name>Deng D.</name></creator><creator><name>Yu B.</name></creator><creator><name>Zijlstra A.</name></creator><date role="Updated">2024-11-06T20:18:17Z</date><date role="Created">2024-02-23T07:04:17Z</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>ob-stars</subject><subject>radio-spectroscopy</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>effective-temperature</subject><subject>stellar-masses</subject><description>Radio observation is crucial to understanding the wind mechanism of OB stars but very scarce. This work estimates the flux at 1450MHz (S1.4GHz) of about 5000 OB stars identified by the LAMOST spectroscopic survey and confirmed by the Gaia astrometric as well as astrophysical measurements. The calculation is performed under the free-free emission mechanism for wind with the mass-loss rate derived from stellar parameters. The estimated S1.4GHz distributes from 10^-11^ to 10^-3^Jy with the peak at about 10^-8^Jy. This implies that the complete SKA-II can detect more than half of them, and some tens of objects are detectable by FAST without considering source confusion. An array of FAST would increase the detectable sample by 2 orders of magnitude.</description><source format="bibcode">2023AJ....166...23H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/23</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/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/146">V/146 : LAMOST DR1 catalogs (Luo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/131">J/AJ/149/131 : Parameters galactic nearby main-sequence stars (Eker+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/484/1838">J/MNRAS/484/1838 : Spatial substructure of Cygnus OB2 (Berlanas+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/495/2738">J/MNRAS/495/2738 : Luminosities 34 slowly pulsating B stars (Pedersen+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/257/54">J/ApJS/257/54 : Early-type star param. from LAMOST LRS &amp; MRS (Guo+, 2021)</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/AJ/166/23</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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32182 32212 32245 32277 32607 32664 32687 32704 32719 36857 40886</spatial><spectral>9.607801192902234e-25 3.916500758235022e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/166/23?format=ascii</footprint><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/166/23/table1</name><description>The S1.4GHz brightest OB stars</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>ID</name><description>[0/4929] Internal index number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>[0/360] Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-10/66] Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Teff</name><description>[1.25/4.1] Effective temperature</description><unit>10000K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logg</name><description>[2.5/4.6] log surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>plx</name><description>[0.07/2.93] Gaia DR3 parallax</description><unit>mas</unit><ucd>pos.parallax.trig</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[339/9400] Distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Bpmag</name><description>[4.29/16.1] Gaia DR3 Blue passband magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rpmag</name><description>[4.48/15.8] Gaia DR3 Red passband magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ABp</name><description>[0/8.44] Extinction in Gaia DR3 Blue passband</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ARp</name><description>[0/4.85] Extinction in Gaia DR3 Red passband</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bp0mag</name><description>[4.29/15.1] Extinction corrected Gaia DR3 Blue passband magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rp0mag</name><description>[4.48/15.3] Extinction corrected Gaia DR3 Red passband magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>(Bp-Rp)0</name><description>[-0.5/-0.1] Extinction correct Bp-Rp color</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BpMAG</name><description>[-6.35/1.92] Absolute Gaia DR3 Blue passband magnitude</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RpMAG</name><description>[-6.02/2.16] Absolute Gaia DR3 Red passband magnitude</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>[4.2/82.3] Stellar mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lum</name><description>[377/2881346] Stellar luminosity</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Mdot</name><description>[0.16/628527] Mass loss rate, 10-6xM{sun}/yr</description><ucd>phys.mass.loss</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[0.002/1550650] Estimated flux at 1450 MHz</description><unit>nJy</unit><ucd>phot.flux.density;em.radio.750-1500MHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BC</name><description>[-6.15/-3.41] Bolometric magnitude</description><unit>mag</unit><ucd>phot.mag.bc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>