<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2023-10-27T09:04:53Z" status="active" updated="2026-07-01T14:00:59Z" version="1.2" 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/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>Ionized clouds in central arcsecond of NGC 1068</title><shortName>J/A+A/678/A206</shortName><identifier>ivo://CDS.VizieR/J/A+A/678/A206</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-n6/lcag</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Vermot P.</name></creator><creator><name>Barna B.</name></creator><creator><name>Ehlerova S.</name></creator><creator><name>Morris M.</name></creator><creator><name>Palous J.</name></creator><creator><name>Wunsch R.</name></creator><date role="Updated">2026-07-01T14:00:59Z</date><date role="Created">2023-10-27T09:04:53Z</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>active-galactic-nuclei</subject><subject>interstellar-medium</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>Several bright emission line regions are observed in the central 100 parsecs of the active galaxy NGC 1068. We aim to determine the properties and ionization mechanism of three regions: the nucleus itself (B), and two clouds located 0.3" and 0.7" North of it (C and D). We have combined SPHERE (0.95-1.65um) and SINFONI (1.5-2.45um) spectra for the three regions B, C and D. We compare these spectra to several CLOUDY photoionization models and to the MAPPINGS III Library of Fast Radiative Shock Models. The emission line spectra of the three regions are almost identical to each other, and contribute to most of the emission line flux in the nuclear region. The emitting media contain multiple phases, the most luminous of which have temperatures ranging from 104.8K to 106K. Central photoionization models can reproduce some features of the spectra, but the fast radiative shock model provides the best fit to the data. The similarity between the three regions indicates that they belong to the same class of objects. Based on our comparisons, we conclude that they are shock regions located where the AGN jet impacts massive molecular clouds.</description><source format="bibcode">2023A&amp;A...678A.206V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/678/A206</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/591/138">J/ApJ/591/138 : Chandra X-ray sources of NGC 1068 (Smith+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/602/A78">J/A+A/602/A78 : NGC1068 interferometric mid-IR measurements</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/613/A3">J/A+A/613/A3 : NGC 1068 deep millimeter spectroscopy observations</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A100">J/A+A/625/A100 : NGC 1068 SPHERE-VLT images (Rouan+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/634/A1">J/A+A/634/A1 : NGC 1068 GRAVITY reconstructed image (GRAVITY+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/634/A125">J/A+A/634/A125 : NGC 1068 nucleus molecular line spectra at 2mm (Qiu+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/660/A83">J/A+A/660/A83 : NGC1068 I-HCN(1-0) and I-HCO+(1-0) maps</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/A+A/678/A206</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/678/A206</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/678/A206</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/678/A206</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/678/A206</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/678/A206</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/678/A206/spb</name><description>Cloud B spectrum</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>lambda</name><description>Wavelength</description><unit>m</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Flux</description><unit>W.m**-2.um**-1</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/678/A206/spc</name><description>Cloud C spectrum</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>lambda</name><description>Wavelength</description><unit>m</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Flux</description><unit>W.m**-2.um**-1</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/678/A206/spd</name><description>Cloud D spectrum</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>lambda</name><description>Wavelength</description><unit>m</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Flux</description><unit>W.m**-2.um**-1</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/678/A206/table1</name><description>Summary of emission lines</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>Line</name><description>Line identification</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>lambda</name><description>Rest wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E</name><description>Ionization energy</description><unit>eV</unit><ucd>phys.energy;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FluxB</name><description>? Cloud B measured flux</description><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_FluxB</name><description>? Cloud B measured flux error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>FluxC</name><description>Cloud C measured flux</description><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FluxC</name><description>Cloud C measured flux error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FluxD</name><description>Cloud D measured flux</description><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_FluxD</name><description>Cloud D measured flux error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/678/A206/tablee1</name><description>Cloud B: Comparison between the observation and the best SHK model</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>Line</name><description>Line Identification</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>lambda</name><description>Rest Wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E</name><description>Ionization Energy</description><unit>eV</unit><ucd>phys.energy;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>Measured flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>Measured flux error</description><unit>1e-18W.m**-2</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FluxMod</name><description>? Model flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/678/A206/tablee2</name><description>Cloud C: Comparison between the observation and the best SHK model</description><column><name>e_Flux</name><description>Measured flux error</description><unit>1e-18W.m**-2</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FluxMod</name><description>? Model flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</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>Line</name><description>Line Identification</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>lambda</name><description>Rest Wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E</name><description>Ionization Energy</description><unit>eV</unit><ucd>phys.energy;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>Measured flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/678/A206/tablee3</name><description>Cloud D: Comparison between the observation and the best SHK model</description><column><name>Line</name><description>Line Identification</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>lambda</name><description>Rest Wavelength</description><unit>nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E</name><description>Ionization Energy</description><unit>eV</unit><ucd>phys.energy;phys.atmol.ionization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>Measured flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>Measured flux error</description><unit>1e-18W.m**-2</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FluxMod</name><description>? Model flux</description><unit>1e-18W.m**-2</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</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></table></schema></tableset></ri:Resource>