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dc.provenanceCONICET-
dc.creatorFolatelli, Gaston-
dc.creatorVan Dyk, Schuyler D.-
dc.creatorKuncarayakti, Hanindyo-
dc.creatorMaeda, Keiichi-
dc.creatorBersten, Melina Cecilia-
dc.creatorNomoto, Ken’ichi-
dc.creatorPignata, Giuliano-
dc.creatorHamuy, Mario-
dc.creatorQuimby, Robert M.-
dc.creatorZheng, Weikang-
dc.creatorFilippenko, Alexei V.-
dc.creatorClubb, Kelsey I.-
dc.creatorSmith, Nathan-
dc.creatorElias Rosa, Nancy-
dc.creatorFoley, Ryan J.-
dc.creatorMiller, Adam A.-
dc.date2018-02-15T14:16:12Z-
dc.date2018-02-15T14:16:12Z-
dc.date2016-06-
dc.date2018-02-07T17:02:20Z-
dc.date.accessioned2019-04-29T15:30:09Z-
dc.date.available2019-04-29T15:30:09Z-
dc.date.issued2016-06-
dc.identifierFolatelli, Gaston; Van Dyk, Schuyler D.; Kuncarayakti, Hanindyo; Maeda, Keiichi; Bersten, Melina Cecilia; et al.; Disappearance of the progenitor of supernova iPTF13bvn; IOP Publishing; Astrophysical Journal; 825; 2; 6-2016; 1-7-
dc.identifier0004-637X-
dc.identifierhttp://hdl.handle.net/11336/36513-
dc.identifierCONICET Digital-
dc.identifierCONICET-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/295290-
dc.descriptionSupernova (SN) iPTF13bvn in NGC 5806 was the first Type Ib SN to have been tentatively associated with a progenitor in pre-explosion images. We performed deep ultraviolet (UV) and optical Hubble Space Telescope observations of the SN site ˜740 days after explosion. We detect an object in the optical bands that is fainter than the pre-explosion object. This dimming is likely not produced by dust absorption in the ejecta; thus, our finding confirms the connection of the progenitor candidate with the SN. The object in our data is likely dominated by the fading SN, implying that the pre-SN flux is mostly due to the progenitor. We compare our revised pre-SN photometry with previously proposed models. Although binary progenitors are favored, models need to be refined. In particular, to comply with our deep UV detection limit, any companion star must be less luminous than a late-O star or substantially obscured by newly formed dust. A definitive progenitor characterization will require further observations to disentangle the contribution of a much fainter SN and its environment.-
dc.descriptionFil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. The University of Tokyo; Japón-
dc.descriptionFil: Van Dyk, Schuyler D.. Infrared Processing and Analysis Center; Estados Unidos-
dc.descriptionFil: Kuncarayakti, Hanindyo. Universidad de Chile; Chile-
dc.descriptionFil: Maeda, Keiichi. The University of Tokyo; Japón-
dc.descriptionFil: Bersten, Melina Cecilia. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica la Plata; Argentina. The University of Tokyo; Japón-
dc.descriptionFil: Nomoto, Ken’ichi. The University of Tokyo; Japón-
dc.descriptionFil: Pignata, Giuliano. Universidad Andrés Bello; Chile-
dc.descriptionFil: Hamuy, Mario. Universidad de Chile; Chile-
dc.descriptionFil: Quimby, Robert M.. The University of Tokyo; Japón-
dc.descriptionFil: Zheng, Weikang. University of California; Estados Unidos-
dc.descriptionFil: Filippenko, Alexei V.. University of California; Estados Unidos-
dc.descriptionFil: Clubb, Kelsey I.. University of California; Estados Unidos-
dc.descriptionFil: Smith, Nathan. University of Arizona; Estados Unidos-
dc.descriptionFil: Elias Rosa, Nancy. Osservatorio Astronomico di Padova; Italia-
dc.descriptionFil: Foley, Ryan J.. University of Illinois at Urbana Champaign; Estados Unidos-
dc.descriptionFil: Miller, Adam A.. Jet Propulsion Laboratory; Estados Unidos-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherIOP Publishing-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2016ApJ...825L..22F-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.3847/2041-8205/825/2/L22-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.source.urihttp://hdl.handle.net/11336/36513-
dc.subjectSupernovae-
dc.subjectStellar evolution-
dc.subjectHydrodynamics-
dc.subjectiPTF13bvn (supernova)-
dc.subjectNGC 5806 (galaxia)-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleDisappearance of the progenitor of supernova iPTF13bvn-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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