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<ri:Resource created="2020-07-22T12:53:21Z" 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>Nitrogen abundances for Be and B stars</title><shortName>J/MNRAS/471/3398</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/471/3398</identifier><altIdentifier>doi:10.26093/cds/vizier.74713398</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ahmed A.</name></creator><creator><name>Sigut T.A.A.</name></creator><date role="Updated">2024-08-17T20:20:26Z</date><date role="Created">2020-07-22T12:53:21Z</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>b-stars</subject><subject>chemical-abundances</subject><subject>effective-temperature</subject><description>Photospheric nitrogen abundances for a sample of 26 Be stars and 16 normal B stars were found using high-resolution spectra from the Magnetism in Massive Stars (MiMeS) spectroscopic survey. Nitrogen abundances were obtained using non-local-thermodynamic-equilibrium equivalent widths and line profiles, and Monte Carlo simulation was used to determine the error bounds of the measured nitrogen abundances due to uncertainties in the adopted stellar parameters, continuum normalization and atomic data. In addition, the effects of gravitational darkening and disc contamination on the measured Be star nitrogen abundances were investigated. About one third of the sample of Be stars and half of the normal B-type stars have nitrogen enrichment that may be due to rotational mixing in these rapidly rotating objects. Corrections for gravitational darkening and disc contamination do not significantly change the overall results for the Be star sample. The average nitrogen abundance of the B and Be star samples coincides with the solar abundance, although the dispersion in the nitrogen abundances is much larger in the Be star sample. The Be star sample also has a significant fraction of sub-solar nitrogen abundance objects that are not present in significant numbers in the B star sample. This may point to yet unresolved systematic errors in the analysis of the Be stars.</description><source format="bibcode">2017MNRAS.471.3398A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/471/3398</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/J/A+A/440/305">J/A+A/440/305 : Fundamental parameters of fast-rotating B stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/252">J/MNRAS/371/252 : Southern B and Be stars (Levenhagen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/501/297">J/A+A/501/297 : Effective temperatures of B Supergiants (Zorec+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/539/A143">J/A+A/539/A143 : Nearby B-stars stellar parameters and abundances</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A12">J/A+A/551/A12 : HD 48977 frequency analysis (Thoul+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A79">J/A+A/550/A79 : H{alpha} and H{beta} lines of northern Be stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/456/2">J/MNRAS/456/2 : MiMeS survey of magnetism in massive stars (Wade+, 2016)</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/MNRAS/471/3398</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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