Gamma Ray Bursts with peculiar temporal asymmetry

Autores
Romero, Gustavo Esteban; Torres, Diego F.; Andruchow, Ileana; Anchordoqui, Luis Alfredo; Link, Bennett
Año de publicación
1999
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Based on the study of temporal asymmetry of 631 gamma ray bursts from the BATSE 3B catalog by Link and Epstein [Ap J 466, 764 (1996)], we identify the population of bursts whose rising times are longer than their decays, thus showing atypical profiles. We analyse their sky distribution, morphology, time-space clustering and other average properties and compare them with those associated with the bulk of the bursts. We show how most of the peculiar bursts analysed are consistent with recent fireball models, but a fraction of bursts (∼ 4 of the total sample) appear to be inconsistent.
Instituto Argentino de Radioastronomía
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Physics
Gamma-ray burst
Population
Asymmetry
Astrophysics
Sky
Astronomy
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/122769
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/122769
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Gamma Ray Bursts with peculiar temporal asymmetryRomero, Gustavo EstebanTorres, Diego F.Andruchow, IleanaAnchordoqui, Luis AlfredoLink, BennettCiencias AstronómicasPhysicsGamma-ray burstPopulationAsymmetryAstrophysicsSkyAstronomyBased on the study of temporal asymmetry of 631 gamma ray bursts from the BATSE 3B catalog by Link and Epstein [Ap J 466, 764 (1996)], we identify the population of bursts whose rising times are longer than their decays, thus showing atypical profiles. We analyse their sky distribution, morphology, time-space clustering and other average properties and compare them with those associated with the bulk of the bursts. We show how most of the peculiar bursts analysed are consistent with recent fireball models, but a fraction of bursts (∼ 4 of the total sample) appear to be inconsistent.Instituto Argentino de RadioastronomíaFacultad de Ciencias Astronómicas y Geofísicas1999-09-23info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf799-806http://sedici.unlp.edu.ar/handle/10915/122769enginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/308/3/799/973665info:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/issn/1365-2966info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/9904107info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.1999.02808.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T11:01:18Zoai:sedici.unlp.edu.ar:10915/122769Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 11:01:18.839SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Gamma Ray Bursts with peculiar temporal asymmetry
title Gamma Ray Bursts with peculiar temporal asymmetry
spellingShingle Gamma Ray Bursts with peculiar temporal asymmetry
Romero, Gustavo Esteban
Ciencias Astronómicas
Physics
Gamma-ray burst
Population
Asymmetry
Astrophysics
Sky
Astronomy
title_short Gamma Ray Bursts with peculiar temporal asymmetry
title_full Gamma Ray Bursts with peculiar temporal asymmetry
title_fullStr Gamma Ray Bursts with peculiar temporal asymmetry
title_full_unstemmed Gamma Ray Bursts with peculiar temporal asymmetry
title_sort Gamma Ray Bursts with peculiar temporal asymmetry
dc.creator.none.fl_str_mv Romero, Gustavo Esteban
Torres, Diego F.
Andruchow, Ileana
Anchordoqui, Luis Alfredo
Link, Bennett
author Romero, Gustavo Esteban
author_facet Romero, Gustavo Esteban
Torres, Diego F.
Andruchow, Ileana
Anchordoqui, Luis Alfredo
Link, Bennett
author_role author
author2 Torres, Diego F.
Andruchow, Ileana
Anchordoqui, Luis Alfredo
Link, Bennett
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Physics
Gamma-ray burst
Population
Asymmetry
Astrophysics
Sky
Astronomy
topic Ciencias Astronómicas
Physics
Gamma-ray burst
Population
Asymmetry
Astrophysics
Sky
Astronomy
dc.description.none.fl_txt_mv Based on the study of temporal asymmetry of 631 gamma ray bursts from the BATSE 3B catalog by Link and Epstein [Ap J 466, 764 (1996)], we identify the population of bursts whose rising times are longer than their decays, thus showing atypical profiles. We analyse their sky distribution, morphology, time-space clustering and other average properties and compare them with those associated with the bulk of the bursts. We show how most of the peculiar bursts analysed are consistent with recent fireball models, but a fraction of bursts (∼ 4 of the total sample) appear to be inconsistent.
Instituto Argentino de Radioastronomía
Facultad de Ciencias Astronómicas y Geofísicas
description Based on the study of temporal asymmetry of 631 gamma ray bursts from the BATSE 3B catalog by Link and Epstein [Ap J 466, 764 (1996)], we identify the population of bursts whose rising times are longer than their decays, thus showing atypical profiles. We analyse their sky distribution, morphology, time-space clustering and other average properties and compare them with those associated with the bulk of the bursts. We show how most of the peculiar bursts analysed are consistent with recent fireball models, but a fraction of bursts (∼ 4 of the total sample) appear to be inconsistent.
publishDate 1999
dc.date.none.fl_str_mv 1999-09-23
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/122769
url http://sedici.unlp.edu.ar/handle/10915/122769
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/308/3/799/973665
info:eu-repo/semantics/altIdentifier/issn/0035-8711
info:eu-repo/semantics/altIdentifier/issn/1365-2966
info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/9904107
info:eu-repo/semantics/altIdentifier/doi/10.1046/j.1365-8711.1999.02808.x
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
799-806
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.13397

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