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<ri:Resource created="2019-10-30T15:39:48Z" 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>Knots in the deep [FeII]+[SiI] image of the SNR Cas A</title><shortName>J/ApJ/866/139</shortName><identifier>ivo://CDS.VizieR/J/ApJ/866/139</identifier><altIdentifier>doi:10.26093/cds/vizier.18660139</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Koo B.-C.</name></creator><creator><name>Kim H.-J.</name></creator><creator><name>Lee Y.-H.</name></creator><creator><name>Raymond J.C.</name></creator><creator><name>Lee J.-J.</name></creator><creator><name>Yoon S.-C.,Moon D.-S.</name></creator><date role="Updated">2019-10-30T14:54:39Z</date><date role="Created">2019-10-30T15:39:48Z</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>interstellar-medium</subject><subject>supernova-remnants</subject><subject>proper-motions</subject><subject>infrared-sources</subject><subject>astronomical-object-identification</subject><subject>visible-astronomy</subject><subject>radial-velocity</subject><description>We present a long-exposure (~10hr), narrowband image of the supernova (SN) remnant Cassiopeia A (Cas A) centered at 1.644{mu}m emission. The passband contains [FeII] 1.644{mu}m and [SiI] 1.645{mu}m lines, and our "deep [FeII]+[SiI] image" provides an unprecedented panoramic view of Cas A, showing both shocked and unshocked SN ejecta, together with shocked circumstellar medium at subarcsecond (~0.7" or 0.012pc) resolution. The diffuse emission from the unshocked SN ejecta has a form of clumps, filaments, and arcs, and their spatial distribution correlates well with that of the Spitzer [SiII] infrared emission, suggesting that the emission is likely due to [SiI] not [FeII] as in shocked material. The structure of the optically invisible western area of Cas A is clearly seen for the first time. The area is filled with many quasi-stationary flocculi (QSFs) and fragments of the disrupted ejecta shell. We identified 309 knots in the deep [FeII]+[SiI] image and classified them into QSFs and fast-moving knots (FMKs). The comparison with previous optical plates indicates that the lifetime of most QSFs is &gt;~60yr. The total H+He mass of QSFs is ~0.23M_{sun}_, implying that the mass fraction of dense clumps in the progenitor's mass ejection immediately prior to the SN explosion is about 4%-6%. FMKs in the deep [FeII]+[SiI] image mostly correspond to S-rich ejecta knots in optical studies, while those outside the southeastern disrupted ejecta shell appear Fe-rich. The mass of the [FeII] line emitting, shocked dense Fe ejecta is ~3x10^-5^M_{sun}_.</description><source format="bibcode">2018ApJ...866..139K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/866/139</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/ApJ/456/234">J/ApJ/456/234 : Cas A radio knots spectral indices (Anderson+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/267">J/A+A/368/267 : Spatially resolved spectroscopy of Cas A (Maccarone+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/613/343">J/ApJ/613/343 : Cas A knot and filament proper motions (Delaney+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/475/765">J/A+A/475/765 : Fine structure forbidden lines in FeII (Ramsbottom+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/179/195">J/ApJS/179/195 : A catalog of outer ejecta knots in Cas A (Hammell+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A74">J/A+A/536/A74 : FeII forbidden lines radiative transition rates (Deb+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/548/A79">J/A+A/548/A79 : INTEGRAL-OMC optically var. sources (Alfonso-Garzon+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/837/118">J/ApJ/837/118 : NIR knots in the Cas A supernova remnant (Lee+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/612/A110">J/A+A/612/A110 : Cas A LOFAR and VLA images (Arias+, 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/866/139</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/866/139</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/866/139</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/866/139</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/866/139</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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