<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2015-06-15T08:49:33Z" 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>Water and methanol masers in G75.78+0.34</title><shortName>J/ApJ/766/114</shortName><identifier>ivo://CDS.VizieR/J/ApJ/766/114</identifier><altIdentifier>doi:10.26093/cds/vizier.17660114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanchez-Monge A.</name></creator><creator><name>Kurtz S.</name></creator><creator><name>Palau A.</name></creator><creator><name>Estalella R.</name></creator><creator><name>Shepherd D.</name></creator><creator><name>Lizano S.,Franco J.</name></creator><creator><name>Garay G.</name></creator><date role="Updated">2015-07-09T16:36:01Z</date><date role="Created">2015-06-15T08:49:33Z</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>astrophysical-masers</subject><subject>radio-astronomy</subject><subject>radio-continuum-emission</subject><subject>h-ii-regions</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>interstellar-medium</subject><description>We present subarcsecond observations toward the massive star-forming region G75.78+0.34. We used the Very Large Array to study the centimeter continuum and H_2_O and CH_3_OH maser emission, and the Owens Valley Radio Observatory and Submillimeter Array to study the millimeter continuum and recombination lines (H40{alpha} and H30{alpha}). We found radio continuum emission at all wavelengths, coming from three components: (1) a cometary ultracompact (UC) H II region with an electron density ~3.7x10^4^/cm3, excited by a B0 type star, and with no associated dust emission; (2) an almost unresolved UCH II region (EAST), located ~6" to the east of the cometary UCH II region, with an electron density ~1.3x10^5^/cm3, and associated with a compact dust clump detected at millimeter and mid-infrared wavelengths; and (3) a compact source (CORE), located ~2" to the southwest of the cometary arc, with a flux density increasing with frequency, and embedded in a dust condensation of 30M_{sun}_. The CORE source is resolved into two compact and unresolved sources which can be well fit by two homogeneous hypercompact H II regions each one photoionized by a B0.5 zero-age main sequence star, or by free-free radiation from shock-ionized gas resulting from the interaction of a jet/outflow system with the surrounding environment. The spatial distribution and kinematics of water masers close to the CORE-N and S sources, together with excess emission at 4.5{mu}m and the detected dust emission, suggest that the CORE source is a massive protostar driving a jet/outflow.</description><source format="bibcode">2013ApJ...766..114S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/766/114</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/J/other/IJAA/4.571">J/other/IJAA/4.571 : Methanol masers in HII regions (Farmer, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/2">J/ApJ/763/2 : 95GHz methanol masers in molecular outflows (Gan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2391">J/AJ/136/2391 : GLIMPSE Extended Green Objects catalog (Cyganowski+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/685/1005">J/ApJ/685/1005 : Spitzer and high-mass star forming regions (Qiu+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/277">J/ApJS/175/277 : Submillimeter-Continuum SCUBA detections (Di Francesco+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/155/149">J/ApJS/155/149 : CH_3_OH 7_0_-6_1_ A^+^ maser sources (Kurtz+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/133/29">J/A+AS/133/29 : Molecular line survey towards UC HII (Hatchell+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/120/283">J/A+AS/120/283 : Water maser features in HII regions (Hofner+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/111/846">J/AJ/111/846 : Orion HST survey (O'Dell+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/291/943">J/A+A/291/943 : Protostellar cores (Ossenkopf+, 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/ApJ/766/114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/766/114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/766/114</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/766/114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/766/114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/766/114</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/ApJ/766/114/table4 (22GHz water and 44GHz methanol masers in G75.78+0.34)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/766/114/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/766/114/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/766/114/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>305.4332</ra><dec>37.443825</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/14622</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/766/114?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/766/114/table4</name><description>22GHz water and 44GHz methanol masers in G75.78+0.34</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>Mol</name><description>Maser component (H_2_O or CH_3_OH)</description><ucd>meta.id;phys.mol</ucd></column><column><name>RAJ2000</name><description>[20] Hour of right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[37] Degree of declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Spk</name><description>[0.06/122] Peak flux intensity</description><unit>Jy</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vpk</name><description>[-36/14] Peak velocity (LSR)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sdv</name><description>[0.04/220] Integrated intensity</description><unit>Jy.km/s</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Notes</name><description>[ ,1-4HL] Notes (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>