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<ri:Resource created="2024-06-07T11:44:22Z" 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>Does magnetized OB stars produce magnetars ?</title><shortName>J/MNRAS/504/5813</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/504/5813</identifier><altIdentifier>doi:10.26093/cds/vizier.75045813</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Makarenko E.I</name></creator><creator><name>Igoshev A.P</name></creator><creator><name>Kholtygin A.F</name></creator><date role="Updated">2024-11-06T20:33:44Z</date><date role="Created">2024-06-07T11:44:22Z</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>magnetic-fields</subject><subject>neutron-stars</subject><subject>x-ray-sources</subject><subject>photometry</subject><description>Stars of spectral types O and B produce neutron stars (NSs) after supernova explosions. Most of NSs are strongly magnetized including normal radio pulsars with B {prop.to} 1012 G and magnetars with B {prop.to} 10^14^ G. A fraction of 7-12 per cent of massive stars are also magnetized with B {prop.to} 103 G and some are weakly magnetized with B {prop.to} 1 G. It was suggested that magnetic fields of NSs could be the fossil remnants of magnetic fields of their progenitors. This work is dedicated to study this hypothesis. First, we gather all modern precise measurements of surface magnetic fields in O, B, and A stars. Secondly, we estimate parameters for lognormal distribution of magnetic fields in B stars and found {mu}B = 2.83 +/- 0.1 log10 (G), {sigma}B = 0.65 +/- 0.09 for strongly magnetized and {mu}B = 0.14 +/- 0.5 log10 (G), {sigma} = 0.7_-0.27_^+0.57^ for weakly magnetized. Third, we assume that the magnetic field of pulsars and magnetars have 2.7-dex difference in magnetic fields and magnetars represent 10 per cent of all young NSs and run population synthesis. We found that it is impossible to simultaneously reproduce pulsars and magnetars populations if the difference in their magnetic fields is 2.7 dex. Therefore, we conclude that the simple fossil origin of the magnetic field is not viable for NSs.</description><source format="bibcode">2021MNRAS.504.5813M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/504/5813</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/psr">B/psr : ATNF Pulsar Catalogue (Manchester+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/6">J/ApJS/212/6 : The McGill magnetar catalog (Olausen+, 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28137 28208 28711 28733 28806 28809 28913 30438 30563 30960 31063 31330 31344 31511 31716 31812 31814 33024 33098 33120 33299 33317 34296 36341 36563 37181 37231 37932 38287 38291 38519 39162 39177 39183 39202 39205 39263 39335 39347 39515 39716 39793 39853 39869 39877 40072 40486 40654 40686 40783 40882 41524 41680 41689 41916 41924 42212 42214 42227 42464 42486-42487 42633 42916 42948 42994 43058 43219 43345 43416 43460 43531 43884 44110 44310 44316 44468 44844 46118 47539 47824 48072</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/504/5813?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/504/5813/tablec1</name><description>List of B stars</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Orbital period (Porbital)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>vsini</name><description>? Rotation velocity (vsini)</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_vsini</name><description>? 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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>Name</name><description>A star name (Name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Brms</name><description>Root mean square of magnetic fields (Brms)</description><unit>0.0001T</unit><ucd>phys.magField;phys.mol.dipole.magnetic;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Brms</name><description>Standard deviation of Brms (sigmaB)</description><unit>0.0001T</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_Porb</name><description>[yes no] Flag on the orbital period measurement (f_Porb)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>l_Porb</name><description>Limit flag on Porb (l_Porb)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Porb</name><description>? Orbital period (Porbital)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Refs</name><description>Literature references, in refs.dat file (Ref)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="46*">char</dataType></column></table><table><name>J/MNRAS/504/5813/tablec3</name><description>List of O stars</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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