Disappearance of the progenitor of supernova iPTF13bvn

Autores
Folatelli, Gaston; Van Dyk, Schuyler D.; Kuncarayakti, Hanindyo; Maeda, Keiichi; Bersten, Melina Cecilia; Nomoto, Ken’ichi; Pignata, Giuliano; Hamuy, Mario; Quimby, Robert M.; Zheng, Weikang; Filippenko, Alexei V.; Clubb, Kelsey I.; Smith, Nathan; Elias Rosa, Nancy; Foley, Ryan J.; Miller, Adam A.
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Supernova (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.
Fil: 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
Fil: Van Dyk, Schuyler D.. Infrared Processing and Analysis Center; Estados Unidos
Fil: Kuncarayakti, Hanindyo. Universidad de Chile; Chile
Fil: Maeda, Keiichi. The University of Tokyo; Japón
Fil: 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
Fil: Nomoto, Ken’ichi. The University of Tokyo; Japón
Fil: Pignata, Giuliano. Universidad Andrés Bello; Chile
Fil: Hamuy, Mario. Universidad de Chile; Chile
Fil: Quimby, Robert M.. The University of Tokyo; Japón
Fil: Zheng, Weikang. University of California; Estados Unidos
Fil: Filippenko, Alexei V.. University of California; Estados Unidos
Fil: Clubb, Kelsey I.. University of California; Estados Unidos
Fil: Smith, Nathan. University of Arizona; Estados Unidos
Fil: Elias Rosa, Nancy. Osservatorio Astronomico di Padova; Italia
Fil: Foley, Ryan J.. University of Illinois at Urbana Champaign; Estados Unidos
Fil: Miller, Adam A.. Jet Propulsion Laboratory; Estados Unidos
Materia
Supernovae
Stellar evolution
Hydrodynamics
iPTF13bvn (supernova)
NGC 5806 (galaxia)
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/36513
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/36513
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Disappearance of the progenitor of supernova iPTF13bvnFolatelli, GastonVan Dyk, Schuyler D.Kuncarayakti, HanindyoMaeda, KeiichiBersten, Melina CeciliaNomoto, Ken’ichiPignata, GiulianoHamuy, MarioQuimby, Robert M.Zheng, WeikangFilippenko, Alexei V.Clubb, Kelsey I.Smith, NathanElias Rosa, NancyFoley, Ryan J.Miller, Adam A.SupernovaeStellar evolutionHydrodynamicsiPTF13bvn (supernova)NGC 5806 (galaxia)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Supernova (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.Fil: 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; JapónFil: Van Dyk, Schuyler D.. Infrared Processing and Analysis Center; Estados UnidosFil: Kuncarayakti, Hanindyo. Universidad de Chile; ChileFil: Maeda, Keiichi. The University of Tokyo; JapónFil: 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; JapónFil: Nomoto, Ken’ichi. The University of Tokyo; JapónFil: Pignata, Giuliano. Universidad Andrés Bello; ChileFil: Hamuy, Mario. Universidad de Chile; ChileFil: Quimby, Robert M.. The University of Tokyo; JapónFil: Zheng, Weikang. University of California; Estados UnidosFil: Filippenko, Alexei V.. University of California; Estados UnidosFil: Clubb, Kelsey I.. University of California; Estados UnidosFil: Smith, Nathan. University of Arizona; Estados UnidosFil: Elias Rosa, Nancy. Osservatorio Astronomico di Padova; ItaliaFil: Foley, Ryan J.. University of Illinois at Urbana Champaign; Estados UnidosFil: Miller, Adam A.. Jet Propulsion Laboratory; Estados UnidosIOP Publishing2016-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/36513Folatelli, 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; 1-70004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2016ApJ...825L..22Finfo:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8205/825/2/L22info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:08Zoai:ri.conicet.gov.ar:11336/36513instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:33:08.457CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Disappearance of the progenitor of supernova iPTF13bvn
title Disappearance of the progenitor of supernova iPTF13bvn
spellingShingle Disappearance of the progenitor of supernova iPTF13bvn
Folatelli, Gaston
Supernovae
Stellar evolution
Hydrodynamics
iPTF13bvn (supernova)
NGC 5806 (galaxia)
title_short Disappearance of the progenitor of supernova iPTF13bvn
title_full Disappearance of the progenitor of supernova iPTF13bvn
title_fullStr Disappearance of the progenitor of supernova iPTF13bvn
title_full_unstemmed Disappearance of the progenitor of supernova iPTF13bvn
title_sort Disappearance of the progenitor of supernova iPTF13bvn
dc.creator.none.fl_str_mv Folatelli, Gaston
Van Dyk, Schuyler D.
Kuncarayakti, Hanindyo
Maeda, Keiichi
Bersten, Melina Cecilia
Nomoto, Ken’ichi
Pignata, Giuliano
Hamuy, Mario
Quimby, Robert M.
Zheng, Weikang
Filippenko, Alexei V.
Clubb, Kelsey I.
Smith, Nathan
Elias Rosa, Nancy
Foley, Ryan J.
Miller, Adam A.
author Folatelli, Gaston
author_facet Folatelli, Gaston
Van Dyk, Schuyler D.
Kuncarayakti, Hanindyo
Maeda, Keiichi
Bersten, Melina Cecilia
Nomoto, Ken’ichi
Pignata, Giuliano
Hamuy, Mario
Quimby, Robert M.
Zheng, Weikang
Filippenko, Alexei V.
Clubb, Kelsey I.
Smith, Nathan
Elias Rosa, Nancy
Foley, Ryan J.
Miller, Adam A.
author_role author
author2 Van Dyk, Schuyler D.
Kuncarayakti, Hanindyo
Maeda, Keiichi
Bersten, Melina Cecilia
Nomoto, Ken’ichi
Pignata, Giuliano
Hamuy, Mario
Quimby, Robert M.
Zheng, Weikang
Filippenko, Alexei V.
Clubb, Kelsey I.
Smith, Nathan
Elias Rosa, Nancy
Foley, Ryan J.
Miller, Adam A.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Supernovae
Stellar evolution
Hydrodynamics
iPTF13bvn (supernova)
NGC 5806 (galaxia)
topic Supernovae
Stellar evolution
Hydrodynamics
iPTF13bvn (supernova)
NGC 5806 (galaxia)
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Supernova (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.
Fil: 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
Fil: Van Dyk, Schuyler D.. Infrared Processing and Analysis Center; Estados Unidos
Fil: Kuncarayakti, Hanindyo. Universidad de Chile; Chile
Fil: Maeda, Keiichi. The University of Tokyo; Japón
Fil: 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
Fil: Nomoto, Ken’ichi. The University of Tokyo; Japón
Fil: Pignata, Giuliano. Universidad Andrés Bello; Chile
Fil: Hamuy, Mario. Universidad de Chile; Chile
Fil: Quimby, Robert M.. The University of Tokyo; Japón
Fil: Zheng, Weikang. University of California; Estados Unidos
Fil: Filippenko, Alexei V.. University of California; Estados Unidos
Fil: Clubb, Kelsey I.. University of California; Estados Unidos
Fil: Smith, Nathan. University of Arizona; Estados Unidos
Fil: Elias Rosa, Nancy. Osservatorio Astronomico di Padova; Italia
Fil: Foley, Ryan J.. University of Illinois at Urbana Champaign; Estados Unidos
Fil: Miller, Adam A.. Jet Propulsion Laboratory; Estados Unidos
description Supernova (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.
publishDate 2016
dc.date.none.fl_str_mv 2016-06
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/36513
Folatelli, 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
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/36513
identifier_str_mv Folatelli, 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
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://adsabs.harvard.edu/abs/2016ApJ...825L..22F
info:eu-repo/semantics/altIdentifier/doi/10.3847/2041-8205/825/2/L22
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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