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<ri:Resource created="2019-02-12T06:21:27Z" 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>A study of the H{alpha} variability of Be stars</title><shortName>J/AJ/156/61</shortName><identifier>ivo://CDS.VizieR/J/AJ/156/61</identifier><altIdentifier>doi:10.26093/cds/vizier.51560061</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dimitrov D.P.</name></creator><creator><name>Kjurkchieva D.P.</name></creator><creator><name>Ivanov E.I.</name></creator><date role="Updated">2020-01-17T10:40:46Z</date><date role="Created">2019-02-12T06:21:27Z</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>open-star-clusters</subject><subject>stellar-associations</subject><subject>infrared-photometry</subject><subject>be-stars</subject><subject>stellar-spectral-types</subject><subject>radial-velocity</subject><subject>proper-motions</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><subject>line-intensities</subject><subject>stellar-distance</subject><description>This paper presents the results of 4 years of high-resolution spectral observations of 69 emission-line stars, 54 of them being newly discovered sources. We classified the stars on the basis of their position in the two-color IR diagram and some additional criteria: shape and width of the H{alpha} profile, presence of He lines, proper motion and parallax, membership to open cluster and associations. Sixty of our targets turned out to be Be stars. We also found four late giants, four pre-MS stars, and one late dwarf. The H{alpha} emission profiles of our Be stars range from single peaked to typical shell profiles that can also be highly asymmetric or single-peaked profiles with a narrow absorption core. The emission profiles appear almost constant with time or highly variable in intensity and in their V/R ratio. The detected long-term variability of the H{alpha} emission is important for investigating the on/off switch phenomenon of Be stars. Our study led to an increase of the number of the emission-line stars of 16 open clusters.</description><source format="bibcode">2018AJ....156...61D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/61</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/V/125">V/125 : Photometry and Spectroscopy for Luminous Stars (Reed 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/317">I/317 : The PPMXL Catalog (Roeser+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/322">I/322 : UCAC4 Catalogue (Zacharias+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/454/151">J/ApJ/454/151 : OB Associations of the Northern Milky Way (Massey+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RMxAA/33.83">J/other/RMxAA/33.83 : NGC 129 positions and proper motions (Stock+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/376/144">J/A+A/376/144 : BV(RI)_C_H{alpha} photometry of NGC 663 (Pigulski+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/2254">J/AJ/124/2254 : Speckle interferometry at USNO. 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