An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova

Autores
Della Valle, M.; Chincarini, G.; Panagia, N.; Tagliaferri, G.; Malesani, D.; Testa, V.; Fugazza, D.; Campana, S.; Covino, S.; Mangano, V.; Antonelli, L. A.; D'Avanzo, P.; Hurley, K.; Mirabel Miquele, Igor Felix; Pellizza González, Leonardo Javier; Piranomonte, S.; Stella, L.
Año de publicación
2006
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ~2s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 060614, one of the closest GRBs discovered, consisted of a 5-s hard spike followed by softer, brighter emission that lasted for ~100s (refs 8, 9). Here we report deep optical observations of GRB 060614 showing no emerging supernova with absolute visual magnitude brighter than MV=-13.7. Any supernova associated with GRB 060614 was therefore at least 100 times fainter, at optical wavelengths, than the other supernovae associated with GRBs. This demonstrates that some long-lasting GRBs can either be associated with a very faint supernova or produced by different phenomena.
Fil: Della Valle, M.. Osservatorio Astrofisico di Arcetri; Italia
Fil: Chincarini, G.. Osservatorio Astronomico di Brera; Italia
Fil: Panagia, N.. Space Telescope Science Institute; Estados Unidos
Fil: Tagliaferri, G.. Osservatorio Astronomico di Brera; Italia
Fil: Malesani, D.. International School for Advanced Studies; Italia
Fil: Testa, V.. Osservatorio Astronomico di Roma; Italia
Fil: Fugazza, D.. Osservatorio Astronomico di Brera; Italia
Fil: Campana, S.. Osservatorio Astronomico di Brera; Italia
Fil: Covino, S.. Osservatorio Astronomico di Brera; Italia
Fil: Mangano, V.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Antonelli, L. A.. Osservatorio Astronomico di Roma; Italia
Fil: D'Avanzo, P.. Osservatorio Astronomico di Brera; Italia
Fil: Hurley, K.. University Of California Berkeley; Estados Unidos
Fil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Piranomonte, S.. Osservatorio Astronomico di Roma; Italia
Fil: Stella, L.. Osservatorio Astronomico di Roma; Italia
Materia
GAMMA RAYS: BURSTS
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:11336/21203
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/21203
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling An enigmatic long-lasting γ-ray burst not accompanied by a bright supernovaDella Valle, M.Chincarini, G.Panagia, N.Tagliaferri, G.Malesani, D.Testa, V.Fugazza, D.Campana, S.Covino, S.Mangano, V.Antonelli, L. A.D'Avanzo, P.Hurley, K.Mirabel Miquele, Igor FelixPellizza González, Leonardo JavierPiranomonte, S.Stella, L.GAMMA RAYS: BURSTShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ~2s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 060614, one of the closest GRBs discovered, consisted of a 5-s hard spike followed by softer, brighter emission that lasted for ~100s (refs 8, 9). Here we report deep optical observations of GRB 060614 showing no emerging supernova with absolute visual magnitude brighter than M<sub>V</sub>=-13.7. Any supernova associated with GRB 060614 was therefore at least 100 times fainter, at optical wavelengths, than the other supernovae associated with GRBs. This demonstrates that some long-lasting GRBs can either be associated with a very faint supernova or produced by different phenomena.Fil: Della Valle, M.. Osservatorio Astrofisico di Arcetri; ItaliaFil: Chincarini, G.. Osservatorio Astronomico di Brera; ItaliaFil: Panagia, N.. Space Telescope Science Institute; Estados UnidosFil: Tagliaferri, G.. Osservatorio Astronomico di Brera; ItaliaFil: Malesani, D.. International School for Advanced Studies; ItaliaFil: Testa, V.. Osservatorio Astronomico di Roma; ItaliaFil: Fugazza, D.. Osservatorio Astronomico di Brera; ItaliaFil: Campana, S.. Osservatorio Astronomico di Brera; ItaliaFil: Covino, S.. Osservatorio Astronomico di Brera; ItaliaFil: Mangano, V.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; ItaliaFil: Antonelli, L. A.. Osservatorio Astronomico di Roma; ItaliaFil: D'Avanzo, P.. Osservatorio Astronomico di Brera; ItaliaFil: Hurley, K.. University Of California Berkeley; Estados UnidosFil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Piranomonte, S.. Osservatorio Astronomico di Roma; ItaliaFil: Stella, L.. Osservatorio Astronomico di Roma; ItaliaNature Publishing Group2006-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/21203Della Valle, M.; Chincarini, G.; Panagia, N.; Tagliaferri, G.; Malesani, D.; et al.; An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova; Nature Publishing Group; Nature; 444; 7122; 12-2006; 1050-10520028-0836CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://www.nature.com/nature/journal/v444/n7122/full/nature05374.html?foxtrotcallback=trueinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0608322info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:24:49Zoai:ri.conicet.gov.ar:11336/21203instacron: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:34982025-10-15 14:24:49.837CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
title An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
spellingShingle An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
Della Valle, M.
GAMMA RAYS: BURSTS
title_short An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
title_full An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
title_fullStr An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
title_full_unstemmed An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
title_sort An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
dc.creator.none.fl_str_mv Della Valle, M.
Chincarini, G.
Panagia, N.
Tagliaferri, G.
Malesani, D.
Testa, V.
Fugazza, D.
Campana, S.
Covino, S.
Mangano, V.
Antonelli, L. A.
D'Avanzo, P.
Hurley, K.
Mirabel Miquele, Igor Felix
Pellizza González, Leonardo Javier
Piranomonte, S.
Stella, L.
author Della Valle, M.
author_facet Della Valle, M.
Chincarini, G.
Panagia, N.
Tagliaferri, G.
Malesani, D.
Testa, V.
Fugazza, D.
Campana, S.
Covino, S.
Mangano, V.
Antonelli, L. A.
D'Avanzo, P.
Hurley, K.
Mirabel Miquele, Igor Felix
Pellizza González, Leonardo Javier
Piranomonte, S.
Stella, L.
author_role author
author2 Chincarini, G.
Panagia, N.
Tagliaferri, G.
Malesani, D.
Testa, V.
Fugazza, D.
Campana, S.
Covino, S.
Mangano, V.
Antonelli, L. A.
D'Avanzo, P.
Hurley, K.
Mirabel Miquele, Igor Felix
Pellizza González, Leonardo Javier
Piranomonte, S.
Stella, L.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GAMMA RAYS: BURSTS
topic GAMMA RAYS: BURSTS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ~2s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 060614, one of the closest GRBs discovered, consisted of a 5-s hard spike followed by softer, brighter emission that lasted for ~100s (refs 8, 9). Here we report deep optical observations of GRB 060614 showing no emerging supernova with absolute visual magnitude brighter than M<sub>V</sub>=-13.7. Any supernova associated with GRB 060614 was therefore at least 100 times fainter, at optical wavelengths, than the other supernovae associated with GRBs. This demonstrates that some long-lasting GRBs can either be associated with a very faint supernova or produced by different phenomena.
Fil: Della Valle, M.. Osservatorio Astrofisico di Arcetri; Italia
Fil: Chincarini, G.. Osservatorio Astronomico di Brera; Italia
Fil: Panagia, N.. Space Telescope Science Institute; Estados Unidos
Fil: Tagliaferri, G.. Osservatorio Astronomico di Brera; Italia
Fil: Malesani, D.. International School for Advanced Studies; Italia
Fil: Testa, V.. Osservatorio Astronomico di Roma; Italia
Fil: Fugazza, D.. Osservatorio Astronomico di Brera; Italia
Fil: Campana, S.. Osservatorio Astronomico di Brera; Italia
Fil: Covino, S.. Osservatorio Astronomico di Brera; Italia
Fil: Mangano, V.. Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia
Fil: Antonelli, L. A.. Osservatorio Astronomico di Roma; Italia
Fil: D'Avanzo, P.. Osservatorio Astronomico di Brera; Italia
Fil: Hurley, K.. University Of California Berkeley; Estados Unidos
Fil: Mirabel Miquele, Igor Felix. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Pellizza González, Leonardo Javier. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Piranomonte, S.. Osservatorio Astronomico di Roma; Italia
Fil: Stella, L.. Osservatorio Astronomico di Roma; Italia
description Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ~2s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 060614, one of the closest GRBs discovered, consisted of a 5-s hard spike followed by softer, brighter emission that lasted for ~100s (refs 8, 9). Here we report deep optical observations of GRB 060614 showing no emerging supernova with absolute visual magnitude brighter than M<sub>V</sub>=-13.7. Any supernova associated with GRB 060614 was therefore at least 100 times fainter, at optical wavelengths, than the other supernovae associated with GRBs. This demonstrates that some long-lasting GRBs can either be associated with a very faint supernova or produced by different phenomena.
publishDate 2006
dc.date.none.fl_str_mv 2006-12
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/11336/21203
Della Valle, M.; Chincarini, G.; Panagia, N.; Tagliaferri, G.; Malesani, D.; et al.; An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova; Nature Publishing Group; Nature; 444; 7122; 12-2006; 1050-1052
0028-0836
CONICET Digital
CONICET
url http://hdl.handle.net/11336/21203
identifier_str_mv Della Valle, M.; Chincarini, G.; Panagia, N.; Tagliaferri, G.; Malesani, D.; et al.; An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova; Nature Publishing Group; Nature; 444; 7122; 12-2006; 1050-1052
0028-0836
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://www.nature.com/nature/journal/v444/n7122/full/nature05374.html?foxtrotcallback=true
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/astro-ph/0608322
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 Nature Publishing Group
publisher.none.fl_str_mv Nature Publishing Group
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 13.22299

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