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<ri:Resource created="2013-07-31T07:50:30Z" 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>NIR spectroscopy of Galactic Wolf-Rayet stars. II.</title><shortName>J/AJ/143/149</shortName><identifier>ivo://CDS.VizieR/J/AJ/143/149</identifier><altIdentifier>doi:10.26093/cds/vizier.51430149</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shara M.M.</name></creator><creator><name>Faherty J.K.</name></creator><creator><name>Zurek D.</name></creator><creator><name>Moffat A.F.J.</name></creator><creator><name>Gerke J.</name></creator><creator><name>Doyon R.,Artigau E.</name></creator><creator><name>Drissen L.</name></creator><date role="Updated">2017-06-21T08:22:11Z</date><date role="Created">2013-07-31T07:50:30Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>Wide-band photometry</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>line-intensities</subject><subject>stellar-spectral-types</subject><description>We are continuing a J, K and narrowband imaging survey of 300{deg}^2^ of the plane of the Galaxy, searching for new Wolf-Rayet (W-R) stars. Our survey spans 150{deg} in Galactic longitude and reaches 1{deg} above and below the Galactic plane. The survey has a useful limiting magnitude of K=15 over most of the observed Galactic plane, and K=14 (due to severe crowding) within a few degrees of the Galactic center. Thousands of emission-line candidates have been detected. In spectrographic follow-ups of 146 relatively bright W-R star candidates, we have re-examined 11 previously known WC and WN stars and discovered 71 new W-R stars, 17 of type WN and 54 of type WC. Our latest image analysis pipeline now picks out W-R stars with a 57% success rate. Star subtype assignments have been confirmed with the K-band spectra and distances approximated using the method of spectroscopic parallax. Some of the new W-R stars are among the most distant known in our Galaxy. The distribution of these new W-R stars is beginning to trace the locations of massive stars along the distant spiral arms of the Milky Way.</description><source format="bibcode">2012AJ....143..149S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/143/149</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/297">I/297 : NOMAD Catalog (Zacharias+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/215">III/215 : 7th Catalog of Galactic Wolf-Rayet stars (van der Hucht, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/143">III/143 : Spectrophotometry of Wolf-Rayet Stars (Torres-Dodgen+ 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/123">J/ApJ/733/123 : The Wolf-Rayet content of M33 (NGC 598) (Neugent+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/518/A29">J/A+A/518/A29 : WR stars distribution in 2 nearby galaxies (Leloudas+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/108/669">J/A+AS/108/669 : IUE spectra of WR stars (Niedzielski+, 1994)</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/143/149</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Equivalent width of CIV 2.076{mu}m emission line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_W(2.076)</name><description>[a] Flag on W(2.076) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W(2.110)</name><description>? Equivalent width of HeI+CIII 2.110{mu}m emission line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_W(2.110)</name><description>[b] Flag on W(2.110) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W(2.165)</name><description>? Equivalent width of HeI 2.165{mu}m emission line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_W(2.165)</name><description>[c] Flag on W(2.165) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W(2.189)</name><description>? Equivalent width of HeII 2.189{mu}m emission line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_W(2.189)</name><description>[d] Flag on W(2.189) (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Ratio</name><description>? ratio of equivalent widths W(2.076/2.110) used to categorize the WC stars</description><ucd>spect.line.intensity;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dm(HeI)</name><description>? Difference from the interpolated continum magnitude for the HeI narrowband filter (2)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dm(CIV)</name><description>? Difference from the interpolated continum magnitude for the CIV narrowband filter (2)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dm(Brg)</name><description>? Difference from the interpolated continum magnitude for the Br{gamma} narrowband filter (2)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dm(HeII)</name><description>? Difference from the interpolated continum magnitude for the HeII narrowband filter (2)</description><unit>mag</unit><ucd>phot.mag;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>