Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?

We use the very simple and successful Cannonball Model (CB) of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the strongly extinct optical AG of the relatively nearby GRB 011121, which were made with ground-based telescopes at early times, and with the HST at later...

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Detalles Bibliográficos
Autores principales: Dado, Shlomo, Dar, Arnon, De Rujula, Alvaro
Lenguaje:eng
Publicado: 2002
Materias:
Astrophysics and Astronomy
Acceso en línea:https://dx.doi.org/10.1086/341749
http://cds.cern.ch/record/544689
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author Dado, Shlomo
Dar, Arnon
De Rujula, Alvaro
author_facet Dado, Shlomo
Dar, Arnon
De Rujula, Alvaro
author_sort Dado, Shlomo
collection CERN
description We use the very simple and successful Cannonball Model (CB) of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the strongly extinct optical AG of the relatively nearby GRB 011121, which were made with ground-based telescopes at early times, and with the HST at later time. We show that GRB 011121 was indeed associated with a 1998bw-like supernova at the GRB's redshift, as we had specifically predicted for this GRB before the supernova could be observed.
id cern-544689
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2002
record_format invenio
spelling cern-5446892023-03-14T18:47:12Zdoi:10.1086/341749http://cds.cern.ch/record/544689engDado, ShlomoDar, ArnonDe Rujula, AlvaroIs there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?Astrophysics and AstronomyWe use the very simple and successful Cannonball Model (CB) of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the strongly extinct optical AG of the relatively nearby GRB 011121, which were made with ground-based telescopes at early times, and with the HST at later time. We show that GRB 011121 was indeed associated with a 1998bw-like supernova at the GRB's redshift, as we had specifically predicted for this GRB before the supernova could be observed.We use the very simple and successful Cannonball Model (CB) of gamma ray bursts (GRBs) and their afterglows (AGs) to analyze the observations of the strongly extinct optical AG of the relatively nearby GRB 011121, which were made with ground-based telescopes at early times, and with the HST at later time. We show that GRB 011121 was indeed associated with a 1998bw-like supernova at the GRB's redshift, as we had specifically predicted for this GRB before the supernova could be observed.astro-ph/0203440CERN-TH-2002-152oai:cds.cern.ch:5446892002-03-25
spellingShingle Astrophysics and Astronomy
Dado, Shlomo
Dar, Arnon
De Rujula, Alvaro
Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
title Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
title_full Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
title_fullStr Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
title_full_unstemmed Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
title_short Is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
title_sort is there a 1998bw-like supernova in the afterglow of gamma ray burst 011121?
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1086/341749
http://cds.cern.ch/record/544689
work_keys_str_mv AT dadoshlomo istherea1998bwlikesupernovaintheafterglowofgammarayburst011121
AT dararnon istherea1998bwlikesupernovaintheafterglowofgammarayburst011121
AT derujulaalvaro istherea1998bwlikesupernovaintheafterglowofgammarayburst011121

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