<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2012-10-20T14:53:41Z" 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>GM 2-4 H_2_ emission-line objects</title><shortName>J/MNRAS/418/1994</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/418/1994</identifier><altIdentifier>doi:10.26093/cds/vizier.74181994</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Khanzadyan T.</name></creator><creator><name>Movsessian T.A.</name></creator><creator><name>Davis C.J.</name></creator><creator><name>Magakian T.Yu.</name></creator><creator><name>Gredel R.,Nikogossian E.H.</name></creator><date role="Updated">2024-07-16T20:11:58Z</date><date role="Created">2012-10-20T14:53:41Z</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>molecular-clouds</subject><subject>infrared-sources</subject><description>We present a multi-wavelength study of the region towards the GM 2-4 nebula and the nearby source IRAS 05373+2340. Our near-infrared H_2_ 1-0 S(1) line observations reveal various shock-excited features which are part of several bipolar outflows. We identify candidates for the driving sources of the outflows from a comparison of the multi-waveband archival data sets and spectral energy distribution (SED) modelling. The SED spectral slope ({alpha}^IRAC^) for all the protostars in the field was then compared with the visual extinction map. This comparison suggests that star formation progresses from north-east to south-west across this region.</description><source format="bibcode">2011MNRAS.418.1994K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/418/1994</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/114">V/114 : MSX6C Infrared Point Source Catalog (Egan+ 2003)</relatedResource><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/II/297">II/297 : AKARI/IRC mid-IR all-sky Survey (ISAS/JAXA, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/18">J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/404/661">J/MNRAS/404/661 : Young stellar outflows near-IR imaging (Varricatt+ 2010)</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/418/1994</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/418/1994</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/418/1994</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/418/1994</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/418/1994</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/418/1994</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/MNRAS/418/1994/table1 (List of MHOs (Molecular Hydrogen emission line Objects) detected in H_2_ 1-0 S(1) (2.122{mu}m))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/418/1994/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/418/1994/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/418/1994/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>85.1015417</ra><dec>23.8529444</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/24189</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/418/1994?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/418/1994/table1</name><description>List of MHOs (Molecular Hydrogen emission line Objects) detected in H_2_ 1-0 S(1) (2.122{mu}m)</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>MHO</name><description>Name (&lt;[KMD2011] MHO NNNA&gt; in Simbad)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">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>Flux</name><description>Flux in H_2_ 1-0 S(1) line at 2.122{mu}m (1)</description><unit>aW.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Notes</name><description>Notes (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column></table><table><name>J/MNRAS/418/1994/tablea1</name><description>Photometric value data base for all IRS objects</description><column><name>l_IRS5</name><description>Limit flag on IRS5</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>apIRS3</name><description>? Aperture for IRS3 in Filter</description><unit>arcsec</unit><ucd>instr.fov</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></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>Filt</name><description>Filter</description><ucd>meta.id;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>l_IRS3</name><description>Limit flag on IRS3</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>IRS3</name><description>? IRS3 magnitude in Filter (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_IRS3</name><description>? rms uncertainty on IRS3</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_IRS4</name><description>Limit flag on IRS4</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>IRS4</name><description>? IRS4 magnitude in Filter (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_IRS4</name><description>? rms uncertainty on IRS4</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>apIRS4</name><description>? Aperture for IRS4 in Filter</description><unit>arcsec</unit><ucd>instr.fov</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>IRS5</name><description>? IRS5 magnitude in Filter (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_IRS5</name><description>? rms uncertainty on IRS5</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>apIRS5</name><description>? Aperture for IRS5 in Filter</description><unit>arcsec</unit><ucd>instr.fov</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>IRS6</name><description>? IRS6 magnitude in Filter (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_IRS6</name><description>? rms uncertainty on IRS6</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>apIRS6</name><description>? Aperture for IRS6 in Filter</description><unit>arcsec</unit><ucd>instr.fov</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>IRS7</name><description>? IRS7 magnitude in Filter (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_IRS7</name><description>? rms uncertainty on IRS7</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>apIRS7</name><description>? Aperture for IRS7 in Filter</description><unit>arcsec</unit><ucd>instr.fov</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Refs</name><description>Data origin (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table></schema></tableset></ri:Resource>