<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2018-10-30T06:56:41Z" 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>Be stars in open clusters with PTF/iPTF. I.</title><shortName>J/AJ/155/91</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/91</identifier><altIdentifier>doi:10.26093/cds/vizier.51550091</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Yu P.-C.</name></creator><creator><name>Yu C.-H.</name></creator><creator><name>Lee C.-D.</name></creator><creator><name>Lin C.-C.</name></creator><creator><name>Hsia C.-H.</name></creator><creator><name>Chang C.-K.,Chen I.-C.</name></creator><creator><name>Ngeow C.-C.</name></creator><creator><name>Ip W.-H.</name></creator><creator><name>Chen W.-P.</name></creator><creator><name>Laher R.</name></creator><creator><name>Surace J.,Kulkarni S.R.</name></creator><date role="Updated">2018-11-30T09:20:49Z</date><date role="Created">2018-10-30T06:56:41Z</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>be-stars</subject><subject>proper-motions</subject><subject>infrared-photometry</subject><description>We conducted a search for Be star candidates in open clusters using H{alpha} imaging photometry of the Palomar Transient Factory Survey to investigate some connections among Be star phenomena, cluster environments, and ages. Stellar members of clusters were identified by spatial distributions, near-infrared magnitudes and colors, and by proper motions. Among 104 open clusters, we identified 96 Be star candidates in 32 clusters; 11 of our candidates have been reported in previous studies. We found that the clusters with age 7.5&lt;log(t(year))=&lt;8.5 tend to have more Be star candidates; there is about a 40% occurrence rate within this age bin. The clusters in this age bin also tend to have a higher Be fraction N(Be)/N(Be+B-type). These results suggest that the environments of young and intermediate clusters are favorable to the formation of Be phenomena. Spatial distribution of Be star candidates with different ages implies that they do not form preferentially in the central regions. Furthermore, we showed that the mid-infrared (MIR) colors of the Be star candidates are similar to known Be stars, which could be caused by free-free emission or bound-free emission. Some Be star candidates might have no circumstellar dust according to their MIR colors. Finally, among 96 Be candidates, we discovered that one Be star candidate FSR 0904-1 exhibits long-term variability on the timescale of ~2000 days with an amplitude of 0.2-0.3 mag, indicating a long timescale of disk evolution.</description><source format="bibcode">2018AJ....155...91Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/91</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/II/313">II/313 : Palomar Transient Factory (PTF) photometric catalog 1.0</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/1216">J/ApJ/700/1216 : Spectroscopy of Be stars in open clusters</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/BASI/39.517">J/other/BASI/39.517 : Spectroscopy of classical Be stars (Mathew+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/158">J/AJ/144/158 : Properties of B and Be stars in h and {chi} Persei</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A53">J/A+A/558/A53 : Milky Way global survey of star clusters. II.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/50">J/AJ/155/50 : WISE photometry of Be stars in young open clusters</relatedResource><relatedResource>http://www.ptf.caltech.edu/ : Palomar Transient Factory survey</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/155/91</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/91</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/91</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/155/91</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/155/91</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/155/91</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/155/91/table1 (Basic Properties of the Cluster Sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/91/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/91/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/91/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>5.514</ra><dec>61.741</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/155/91/BeStars (Basic Properties (table 2) and WISE Photometric Data (table 3) of Be Star Candidates)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/91/BeStars?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/91/BeStars?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/91/BeStars?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>6.363</ra><dec>62.7103139</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/814 6/1267 1297 1299 1302 1325 1330 1335 1380 1385 1446 1458 1464 1476 1653 1757 1783 1839 3040 3058 3059 3143 3147 3168 3169 3170 3227 3254 3261 3312 3362 3384 3584 3593 3597 3608 3609 3611 3615 3654 3659 3660 3712 3713 6307 13309 14322 14631 14688 14690 14696 14749 14751 15121 15366 15368 15412 15501 15622 15671 21918 22199 22207 22216 22217 22218 22245 22246 22249 22260 22261 23621 23632 23633 23663 23674 23760 23761 23763 23765 23766 23768 23840 23850 23936 23950 23972 23976 23980 23982 23986 23994 23995 24032 24333 24344 24350 24359 24361 24427 24465 24472 24491 24496 24497 24503 24508 24510 24527 24553</spatial><spectral>1.3088508223161842e-20 6.513807192489934e-20</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/155/91?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/155/91/table1</name><description>Basic Properties of the Cluster Sample</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><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>Cluster</name><description>Name of cluster</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmRA</name><description>[-6.78/4.47] Proper motion of RA {mu}_{alpha}_cos{delta}</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>[-8.86/2.93] Proper motion of DE {mu}_{delta}_</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[1/2.5] Distance of cluster to the Sun</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logAge</name><description>[6.7/9.6] Logarithm of the cluster age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logAge</name><description>[0.01/0.203]? Uncertainty in logAge</description><unit>log(yr)</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Size</name><description>[2.6/57.1] Size of searching region</description><unit>arcmin</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N(Be)</name><description>[0/14] Number of Be star candidate(s) found in this work</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>K(Be)1</name><description>[1/15]? First known Be star number from literature</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>K(Be)2</name><description>[4]? Second known Be star number from literature</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_K(Be)</name><description>Reference(s) of known Be stars (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>N</name><description>[0/515] Number of B-type star(s) in cluster</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/AJ/155/91/BeStars</name><description>Basic Properties (table 2) and WISE Photometric Data (table 3) of Be Star Candidates</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>Star</name><description>Name of Be star candidate</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>f_Star</name><description>[*] Flag on Star (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>RAJ2000</name><description>Hour of Right Ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Degree of Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>pmRA</name><description>[-10.1/7] Proper motion of RA {mu}_{alpha}_cos{delta}</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>pmDE</name><description>[-9.1/10.3] Proper motion of DE {mu}_{delta}_</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>J-H</name><description>[0.016/0.344] 2MASS (J-H) color index</description><unit>mag</unit><ucd>phot.color;em.IR.J;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>H-Ks</name><description>[0.029/0.331] 2MASS (H-K_s_) color index</description><unit>mag</unit><ucd>phot.color;em.IR.H;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Rmag</name><description>[11.01/15.15] R band magnitude obtained from USNO-B and PTF/iPTF catalogue</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Class</name><description>Object classification adopted from SIMBAD (2)</description><ucd>meta.code.class;src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>W1mag</name><description>[9.174/13.081] WISE W1 (3.4{mu}m) band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_W1mag</name><description>[0.021/0.128] Uncertainty in W1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W2mag</name><description>[8.822/13.147] WISE W2 (4.6{mu}m) band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_W2mag</name><description>[0.019/0.038] Uncertainty in W2mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W3mag</name><description>[7.901/12.061]? WISE W3 (12{mu}m) band magnitude</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W3mag</name><description>[0.018/0.267]? Uncertainty in W3mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logAge</name><description>[6.7/9.22] Logarithm of the host cluster age</description><unit>log(yr)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1-W2</name><description>[-0.134/0.405] WISE W1-W2 color index</description><unit>mag</unit><ucd>phot.color;em.IR;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W2-W3</name><description>[-0.524/1.791]? WISE W2-W3 color index</description><unit>mag</unit><ucd>phot.color;em.IR;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>