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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/21203
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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 Técnicas2025-09-29T09:36:10Zoai: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:34982025-09-29 09:36:11.207CONICET 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) |
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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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1844613132806258688 |
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13.070432 |