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<ri:Resource created="2022-05-30T12:58:51Z" 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>1.87 and 2.07um observations of 3 GC clusters</title><shortName>J/MNRAS/480/1507</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/480/1507</identifier><altIdentifier>doi:10.26093/cds/vizier.74801507</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tanaka M.</name></creator><creator><name>Okumura S.-I.</name></creator><creator><name>Takahashi H.</name></creator><creator><name>Osawa K.</name></creator><creator><name>Motohara K.</name></creator><creator><name>Konishi M.,Tateuchi K.</name></creator><creator><name>Kato N.</name></creator><creator><name>Morokuma T.</name></creator><creator><name>Ohsawa R.</name></creator><creator><name>Koshida S.</name></creator><creator><name>Yoshii Y.,Nishimura Y.</name></creator><date role="Updated">2024-08-18T20:21:01Z</date><date role="Created">2022-05-30T12:58:51Z</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>wolf-rayet-stars</subject><subject>galactic-center</subject><subject>infrared-sources</subject><description>In order to investigate populations of massive stars in massive star clusters, we have constructed a near-infrared image set: narrow bands of 1.87 and 2.07{mu}m and the Ks standard band with miniTAO, a 1-m infrared telescope at Atacama. First, we observed the well-known three massive star clusters near the Galactic Centre. Colour-colour diagrams made from the set of images show clear excess in 1.87{mu}m for WN-type Wolf-Rayet stars, luminous blue variables and Ofpe stars, and also clear excess in 2.07{mu}m for WC-type Wolf-Rayet stars. Our detection in 1.87{mu}m agrees well with the 1.87-{mu}m detection with the Hubble Space Telescope by Dong et al. The 1.87-{mu}m excess of WN stars seems to have a clear correlation to the Ks magnitude. The correlation suggests that the 1.87-{mu}m excess originates in recombination line emission of H and He, and the Ks magnitude includes free-free radiation. Moreover, the Ks magnitude of WN-late stars, excluding the component of the free-free emission, seems to have nearly a common Ks magnitude. However, the colour-colour diagrams also enable us to find the extinction for each star and thus to draw extinction maps. Furthermore, almost all Mira variables reported by Matsunaga et al. are detected in our images. By using the extinction maps, several tens of extremely red sources except for Mira variables are detected. 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J/MNRAS/417/114)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Type</name><description>? Type of the object in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>ID</name><description>Star ID in this study (CNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Ksmag</name><description>Ks magnitude in this study</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n187)</name><description>? Log of the normalized ratio of FN1875/FKs (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(n207)</name><description>Log of the normalized ratio of FN207/FKs (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comment</name><description>? Comment on the 187 excess</description><ucd>meta.note;phot.color.excess</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>_RA</name><description>Positions from Dong et al., 2011, Cat. J/MNRAS/417/114 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from Dong et al., 2011, Cat. J/MNRAS/417/114 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/MNRAS/480/1507/table8</name><description>Correspondence of FN1875 detection with Dong et al. (2011MNRAS.417..114D) for the sources of the Quintuplet cluster area</description><column><name>ID1</name><description>Star ID in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Ks1mag</name><description>? Ks magnitude in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F187/F190</name><description>Ratio F187/F190 in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Type</name><description>? Type of the object in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Ksmag</name><description>Ks magnitude in this study</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n187)</name><description>Log of the normalized ratio of FN1875/FKs (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n207)</name><description>Log of the normalized ratio of FN207/FKs (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comment</name><description>? Comment on the 187 excess</description><ucd>meta.note;phot.color.excess</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>_RA</name><description>Positions from Dong et al., 2011, Cat. J/MNRAS/417/114 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from Dong et al., 2011, Cat. J/MNRAS/417/114 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></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>ID</name><description>Star ID in this study (QNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table><table><name>J/MNRAS/480/1507/table9</name><description>Correspondence of FN1875 detection with Dong et al. (2011MNRAS.417..114D) for the sources of the Arches cluster area</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>ID1</name><description>Star ID in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Ks1mag</name><description>? Ks magnitude in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F187/F190</name><description>Ratio F187/F190 in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Type</name><description>? Type of the object in Dong et al. (2011MNRAS.417..114D, Cat. J/MNRAS/417/114)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>ID</name><description>Star ID in this study (ANNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Ksmag</name><description>Ks magnitude in this study</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n187)</name><description>Log of the normalized ratio of FN1875/FKs (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n207)</name><description>Log of the normalized ratio of FN207/FKs (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comment</name><description>? Comment on the 187 excess</description><ucd>meta.note;phot.color.excess</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>_RA</name><description>Positions from Dong et al., 2011, Cat. J/MNRAS/417/114 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from Dong et al., 2011, Cat. J/MNRAS/417/114 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/MNRAS/480/1507/table11</name><description>Extremely red sources (non-Miras) with T&lt;1000K in the Galactic Centre cluster area</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>Star ID (CNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Ksmag</name><description>Ks-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n187)</name><description>Log of the normalized ratio of FN1875/FKs (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n207)</name><description>Log of the normalized ratio of FN207/FKs (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AAKs</name><description>Average extinction (3)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LAKs</name><description>Local extinction</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comment</name><description>Comment on the source (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column></table><table><name>J/MNRAS/480/1507/table12</name><description>Extremely red sources (non-Miras) with T&lt;1000K in the Quintuplet cluster area</description><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Ksmag</name><description>Ks-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AAKs</name><description>Average extinction (3)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ID</name><description>Star ID (QNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>log(n187)</name><description>Log of the normalized ratio of FN1875/FKs (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n207)</name><description>Log of the normalized ratio of FN207/FKs (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LAKs</name><description>Local extinction</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comment</name><description>Comment on the source (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">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></table><table><name>J/MNRAS/480/1507/table13</name><description>Extremely red sources (non-Miras) with T&lt;1000K in the Arches cluster area</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>Star ID (ANNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Ksmag</name><description>Ks-band magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n187)</name><description>Log of the normalized ratio of FN1875/FKs (1)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(n207)</name><description>Log of the normalized ratio of FN207/FKs (2)</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AAKs</name><description>Average extinction (3)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>LAKs</name><description>Local extinction</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Comment</name><description>Comment on the source (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table></schema></tableset></ri:Resource>