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<ri:Resource created="2019-10-30T09:32:58Z" 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>VLA 22GHz water masers obs. in NGC6334I-MM1</title><shortName>J/ApJ/866/87</shortName><identifier>ivo://CDS.VizieR/J/ApJ/866/87</identifier><altIdentifier>doi:10.26093/cds/vizier.18660087</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brogan C.L.</name></creator><creator><name>Hunter T.R.</name></creator><creator><name>Cyganowski C.J.</name></creator><creator><name>Chibueze J.O.</name></creator><creator><name>Friesen R.K.,Hirota T.</name></creator><creator><name>MacLeod G.C.</name></creator><creator><name>McGuire B.A.</name></creator><creator><name>Sobolev A.M.</name></creator><date role="Updated">2019-10-30T08:35:40Z</date><date role="Created">2019-10-30T09:32:58Z</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><description>We compare multi-epoch sub-arcsecond Very Large Array imaging of the 22GHz water masers toward the massive protocluster NGC 6334I observed before and after the recent outburst of MM1B in (sub)millimeter continuum. Since the outburst, the water maser emission toward MM1 has substantially weakened. Simultaneously, the strong water masers associated with the synchrotron continuum point source CM2 have flared by a mean factor of 6.5 (to 4.2kJy) with highly blueshifted features (up to 70km/s from the LSR) becoming more prominent. The strongest flaring water masers reside 3000au north of MM1B and form a remarkable bow shock pattern whose vertex coincides with CM2 and tail points back to MM1B. Excited OH masers trace a secondary bow shock located ~120au downstream. Atacama Large Millimeter Array images of CS (6-5) reveal a highly collimated north-south structure encompassing the flaring masers to the north and the nonflaring masers to the south seen in projection toward the MM3-UCHII region. Proper motions of the southern water masers over 5.3 years indicate a bulk projected motion of 117km/s southward from MM1B with a dynamical time of 170 years. We conclude that CM2, the water masers, and many of the excited OH masers trace the interaction of the high-velocity bipolar outflow from MM1B with ambient molecular gas. The previously excavated outflow cavity has apparently allowed the radiative energy of the current outburst to propagate freely until terminating at the northern bow shock where it strengthened the masers. Additionally, water masers have been detected toward MM7 for the first time, and a highly collimated CS (6-5) outflow has been detected toward MM4.</description><source format="bibcode">2018ApJ...866...87B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/866/87</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/316">II/316 : UKIDSS-DR6 Galactic Plane Survey (Lucas+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/316/102">J/A+A/316/102 : JHK Photometry in NGC 6334 (Tapia+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/137/43">J/A+AS/137/43 : OH/H2O masers database (Forster+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/432/369">J/A+A/432/369 : Leiden Atomic and Molecular Database (LAMDA) (Schoeier+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/451/1125">J/A+A/451/1125 : Rotational excitation of CS (Lique+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/481/169">J/A+A/481/169 : ATCA 3mm obs. of NGC 6334I and NGC 6334I(N) (Beuther+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/707/1">J/ApJ/707/1 : Water and Methanol masers in NGC 6334I(N) (Brogan+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/130">J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/832/187">J/ApJ/832/187 : ALMA and VLA radio continuum obs. of NGC 6334I (Brogan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/851/L46">J/ApJ/851/L46 : CH_3_OCH_2_OH ALMA detection in NGC 6334I (McGuire+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/854/170">J/ApJ/854/170 : Methanol (CH_3_OH) and OH masers in NGC 6334I (Hunter+, 2018)</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/866/87</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/866/87</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/866/87</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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Hour of right ascension (J2000)</description><ucd>phot.flux;arith.ratio</ucd><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>Assoc</name><description>Association or total</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType><flag>primary</flag></column><column><name>DEJ2000</name><description>? Degree of declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>Flux1</name><description>[4.7/2880]? Integrated flux in the epoch 2011.7</description><unit>Jy.km/s</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flux2</name><description>[1.2/12500]? Integrated flux in the epoch 2017.0</description><unit>Jy.km/s</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Flux3</name><description>[0.2/12600]? Integrated flux in the epoch in the epoch 2017.8</description><unit>Jy.km/s</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>R2/1</name><description>? Integrated flux 2017.0 to 2011.7 ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_R2/1</name><description>Flag on R2/1 (n=new; v=vanished)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>R3/1</name><description>? Integrated flux 2017.8 to 2011.7 ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_R3/1</name><description>Flag on R3/1 (n=new; v=vanished)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>hFlux1</name><description>[2/398]? Highest flux density in the epoch 2011.7</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>hFlux2</name><description>[1/3920]? Highest flux density in the epoch 2017.0</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>hFlux3</name><description>[0.2/4230]? Highest flux density in the epoch 2017.8</description><unit>Jy</unit><ucd>phot.flux.density;em.radio.12-30GHz</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>E1</name><description>Number of fitted properties in epoch 2011.7</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>E2</name><description>Number of fitted properties in epoch 2017.0</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>E3</name><description>Number of fitted properties in epoch 2017.8</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Vlsrmin1</name><description>[-64.5/-8.2]? Minimum LSR velocity in the epoch 2011.7</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vlsrmin2</name><description>[-24.3/8.8]? Minimum LSR velocity in the epoch 2017.0</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vlsrmin3</name><description>[-8/9.8]? Minimum LSR velocity in the epoch 2017.8</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.min</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VlsrPk1</name><description>[-62/2.8]? Peak LSR velocity in the epoch 2011.7</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VlsrPk2</name><description>[-59/4]? Peak LSR velocity in the epoch 2017.0</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VlsrPk3</name><description>[-9/9]? Peak LSR velocity in the epoch 2017.8</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vlsrmax1</name><description>[-78/3.3]? Maximum LSR velocity in the epoch 2011.7</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vlsrmax2</name><description>[-60.8/8.3]? Maximum LSR velocity in the epoch 2017.0</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Vlsrmax3</name><description>[-59.8/14]? 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