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GRB 110205A: Anatomy of a long gamma-ray burst
Gendre B., Atteia J.-L., Boër M., Colas F., Klotz A., Kugel F., Laas-Bourez M., Rinner C., Strajnic J., Stratta G. et al
Astrophysical Journal 748, 1 (2012) article id. 59 - http://hal.archives-ouvertes.fr/hal-00685018
Articles dans des revues avec comité de lecture
Physique/Astrophysique/Phénomènes cosmiques de haute energie
Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie
GRB 110205A: Anatomy of a long gamma-ray burst
Bruce Gendre 1, Jean-Luc Atteia 2, Michel Boër 3, François Colas 4, Alain Klotz 2, François Kugel 5, Myrtille Laas-Bourez 6, Claudine Rinner 5, Jean Strajnic 7, Giulia Stratta 1, Frédéric Vachier 4
1 :  ASI Science Data Center (ASDC)
Italian Space Agency
via Galileo Galilei, 00044 Frascati
Italie
2 :  Institut de recherche en astrophysique et planétologie (IRAP)
CNRS : UMR5277 – Université Paul Sabatier [UPS] - Toulouse III – Observatoire Midi-Pyrénées
France
3 :  Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS)
http://artemis.oca.eu
Université Nice Sophia Antipolis [UNS] – CNRS : UMR7250 – Observatoire de la Côte d'Azur – INSU
Bd de l'Observatoire BP 4229 06304 NICE CEDEX 4
France
4 :  Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE)
http://www.imcce.fr/
CNRS : UMR8028 – INSU – Observatoire de Paris – Université Pierre et Marie Curie (UPMC) - Paris VI – Université Lille I - Sciences et technologies
77 av Denfert-Rochereau 75014 Paris
France
5 :  Observatoire Chante-Perdrix
Observatoire Chante-Perdrix
Dauban, 04150 Banon
France
6 :  School of Physics, University of Western Australia
University of Western Australia
M013 Crawley WA 6009
Australie
7 :  Observatoire de Haute-Provence (OHP)
http://www.obs-hp.fr
CNRS : USR2207 – INSU – Université de Provence - Aix-Marseille I
04870 ST MICHEL L OBSERVATOIRE
France
The Swift burst GRB 110205A was a very bright burst visible in the Northern hemisphere. GRB 110205A was intrinsically long and very energetic and it occurred in a low-density interstellar medium environment, leading to delayed afterglow emission and a clear temporal separation of the main emitting components: prompt emission, reverse shock, and forward shock. Our observations show several remarkable features of GRB 110205A : the detection of prompt optical emission strongly correlated with the BAT light curve, with no temporal lag between the two ; the absence of correlation of the X-ray emission compared to the optical and high energy gamma-ray ones during the prompt phase ; and a large optical re-brightening after the end of the prompt phase, that we interpret as a signature of the reverse shock. Beyond the pedagogical value offered by the excellent multi-wavelength coverage of a GRB with temporally separated radiating components, we discuss several questions raised by our observations: the nature of the prompt optical emission and the spectral evolution of the prompt emission at high-energies (from 0.5 keV to 150 keV) ; the origin of an X-ray flare at the beginning of the forward shock; and the modeling of the afterglow, including the reverse shock, in the framework of the classical fireball model.
Anglais
10/01/2012

Astrophysical Journal (Astrophys. J.)
Publisher American Astronomical Society
ISSN 0004-637X 
internationale
03/2012
748
1
article id. 59

gamma-ray burst: individual: GRB 110205A
21 pages, 5 figures. The original publication is available at http://iopscience.iop.org/0004-637X.

Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1110.0734