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<ri:Resource created="2021-11-12T06:42:17Z" status="active" updated="2025-05-19T09:50:00Z" 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>Spectra of SN 2017eaw 545 &amp; 900 days after explosion</title><shortName>J/ApJ/900/11</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/11</identifier><altIdentifier>doi:10.26093/cds/vizier.19000011</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Weil K.E.</name></creator><creator><name>Fesen R.A.</name></creator><creator><name>Patnaude D.J.</name></creator><creator><name>Milisavljevic D.</name></creator><date role="Updated">2022-03-14T07:13:15Z</date><date role="Created">2021-11-12T06:42:17Z</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>supernovae</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>SN 2017eaw, the tenth supernova observed in NGC6946, was a normal Type II-P supernova with an estimated 11-13M{sun} red supergiant progenitor. Here we present nebular-phase spectra of SN 2017eaw at +545 and +900days post-max, extending approximately 50-400days past the epochs of previously published spectra. While the +545day spectrum is similar to spectra taken between days +400 and +493, the +900day spectrum shows dramatic changes both in spectral features and emission-line profiles. The H{alpha} emission is flat-topped and boxlike with sharp blue and red profile velocities of ~-8000 and +7500km/s. These late-time spectral changes indicate strong circumstellar interaction with a mass-loss shell, expelled ~1700yr before explosion. SN 2017eaw's +900day spectrum is similar to those seen for SN2004et and SN2013ej observed 2-3yr after explosion. We discuss the importance of late-time monitoring of bright SNeII-P and the nature of presupernova mass-loss events for SNII-P evolution.</description><source format="bibcode">2020ApJ...900...11W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/11</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/MNRAS/372/1315">J/MNRAS/372/1315 : UBVRI photometry of SN 2004et (Sahu+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/395/1409">J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/553/A104">J/A+A/553/A104 : LHA 120-N49 supernova remnant maps (Melnik+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/438/L101">J/MNRAS/438/L101 : First month on SN 2013ej (Valenti+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/449/1876">J/MNRAS/449/1876 : Photometric observations of SN PTF11iqb (Smith+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/459/3939">J/MNRAS/459/3939 : Type II supernova light curves (Valenti+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/18">J/AJ/156/18 : APOGEE DR14 Binary comp. evolved stars (Price-Whelan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/885/43">J/ApJ/885/43 : UBVRI &amp; ugriz photo. of supernova SN 2017gmr (Andrews+,2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/487/832">J/MNRAS/487/832 : BVRI photometry of the Type II-P SN 2017eaw (Buta+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/875/85">J/ApJ/875/85 : Optical search SNRs in NGC6946 with WIYN &amp; GMOS (Long+,2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/875/136">J/ApJ/875/136 : BVRI, spectra &amp; IR obs. type II-P SN2017eaw (Van Dyk+, 2019)</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/900/11</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/900/11</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/900/11</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/900/11</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/900/11</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/900/11</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>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/900/11/figure1</name><description>Combined table from original tables</description><column><name>Flux</name><description>Flux in erg/cm2/s/Angstrom (1)</description><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></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>Time</name><description>Time after explosion</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Wave</name><description>Rest Wavelength in Angstroms (1)</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>