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<ri:Resource created="2021-03-08T07:40:12Z" 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>CfA, CSP, BSP and LOSS spec. &amp; phot. of SNe Ia</title><shortName>J/ApJ/882/120</shortName><identifier>ivo://CDS.VizieR/J/ApJ/882/120</identifier><altIdentifier>doi:10.26093/cds/vizier.18820120</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang X.</name></creator><creator><name>Chen J.</name></creator><creator><name>Wang L.</name></creator><creator><name>Hu M.</name></creator><creator><name>Xi G.</name></creator><creator><name>Yang Yi</name></creator><creator><name>Zhao X.</name></creator><creator><name>Li W.</name></creator><date role="Updated">2021-07-05T08:29:37Z</date><date role="Created">2021-03-08T07:40:12Z</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>line-intensities</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>surveys</subject><description>SNe Ia play key roles in revealing the accelerating expansion of the universe, but our knowledge of their progenitors is still very limited. Here we report the discovery of a rigid dichotomy in circumstellar (CS) environments around two subclasses of SNe Ia as defined by their distinct photospheric velocities. For the SNe Ia with high photospheric velocities (HVs), we found a significant excess flux in blue light 60-100 days past maximum, while this phenomenon is absent for SNe with normal photospheric velocity. This blue excess can be attributed to light echoes by circumstellar dust located at a distance of about (1-2)x10^17^cm from the HV subclass. Moreover, we also found that the HV SNe Ia show systematically evolving NaI absorption line by performing a systematic search of variable NaI absorption lines in spectra of all SNe Ia, whereas this evolution is rarely seen in normal ones. The evolving NaI absorption can be modeled in terms of photoionization model, with the location of the gas clouds at a distance of about 2x10^17^cm, in striking agreement with the location of CS dust inferred from B-band light-curve excess. These observations show clearly that the progenitors of HV subclass are likely from single-degenerate progenitor system (i.e., symbiotic binary), while the NV subclass may arise from double-degenerate system.</description><source format="bibcode">2019ApJ...882..120W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/882/120</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/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/2408">J/AJ/112/2408 : Light Curves of 29 SNe (Hamuy+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/627/579">J/ApJ/627/579 : Photometry of variables in NGC 3370 (Riess+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/527">J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/377/1531">J/MNRAS/377/1531 : Opt. &amp; infrared photometry of SN 2004eo (Pastorello+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/1598">J/AJ/135/1598 : Optical spectroscopy of type Ia supernovae (Matheson+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/687/1201">J/ApJ/687/1201 : SN and LGRB locations in their host galaxies (Kelly+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/331">J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/1097">J/ApJ/700/1097 : Light curve parameters of SN Ia (Hicken+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/L139">J/ApJ/699/L139 : Spectral parameters of SNe Ia (Wang+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/519">J/AJ/139/519 : Carnegie supernova project. 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