GRB 110205A: ANATOMY OF A LONG GAMMA-RAY BURST
Identifieur interne : 005C30 ( Main/Exploration ); précédent : 005C29; suivant : 005C31GRB 110205A: ANATOMY OF A LONG GAMMA-RAY BURST
Auteurs : B. Gendre [Italie] ; J. L. Atteia [France] ; M. Boër [France] ; F. Colas [France] ; A. Klotz [France] ; F. Kugel [France] ; M. Laas-Bourez [Australie] ; C. Rinner [France] ; J. Strajnic [France] ; G. Stratta [Italie] ; F. Vachier [France]Source :
- The Astrophysical journal [ 0004-637X ] ; 2012.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
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 Burst Alert Telescope 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 gamma-ray burst 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.
Affiliations:
- Australie, France, Italie
- Midi-Pyrénées, Occitanie (région administrative), Île-de-France
- Paris, Toulouse
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Le document en format XML
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<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Afterglow</term>
<term>Brightening</term>
<term>Correlations</term>
<term>Cosmic gamma sources</term>
<term>Energetics</term>
<term>Fireball model</term>
<term>Gamma radiation</term>
<term>Gamma ray burst</term>
<term>Interstellar matter</term>
<term>Light curves</term>
<term>Light emission</term>
<term>Modelling</term>
<term>Northern hemisphere</term>
<term>X ray emission</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Sursaut Rγ</term>
<term>Hémisphère Nord</term>
<term>Energétique</term>
<term>Matière interstellaire</term>
<term>Postluminescence</term>
<term>Emission optique</term>
<term>Courbe lumière</term>
<term>Corrélation</term>
<term>Emission RX</term>
<term>Rayonnement gamma</term>
<term>Renforcement brillance</term>
<term>Modélisation</term>
<term>Modèle boule feu</term>
<term>Source gamma cosmique</term>
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<front><div type="abstract" xml:lang="en">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 Burst Alert Telescope 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 gamma-ray burst 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.</div>
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<region><li>Midi-Pyrénées</li>
<li>Occitanie (région administrative)</li>
<li>Île-de-France</li>
</region>
<settlement><li>Paris</li>
<li>Toulouse</li>
</settlement>
</list>
<tree><country name="Italie"><noRegion><name sortKey="Gendre, B" sort="Gendre, B" uniqKey="Gendre B" first="B." last="Gendre">B. Gendre</name>
</noRegion>
<name sortKey="Stratta, G" sort="Stratta, G" uniqKey="Stratta G" first="G." last="Stratta">G. Stratta</name>
</country>
<country name="France"><region name="Occitanie (région administrative)"><name sortKey="Atteia, J L" sort="Atteia, J L" uniqKey="Atteia J" first="J. L." last="Atteia">J. L. Atteia</name>
</region>
<name sortKey="Atteia, J L" sort="Atteia, J L" uniqKey="Atteia J" first="J. L." last="Atteia">J. L. Atteia</name>
<name sortKey="Boer, M" sort="Boer, M" uniqKey="Boer M" first="M." last="Boër">M. Boër</name>
<name sortKey="Colas, F" sort="Colas, F" uniqKey="Colas F" first="F." last="Colas">F. Colas</name>
<name sortKey="Klotz, A" sort="Klotz, A" uniqKey="Klotz A" first="A." last="Klotz">A. Klotz</name>
<name sortKey="Klotz, A" sort="Klotz, A" uniqKey="Klotz A" first="A." last="Klotz">A. Klotz</name>
<name sortKey="Kugel, F" sort="Kugel, F" uniqKey="Kugel F" first="F." last="Kugel">F. Kugel</name>
<name sortKey="Rinner, C" sort="Rinner, C" uniqKey="Rinner C" first="C." last="Rinner">C. Rinner</name>
<name sortKey="Strajnic, J" sort="Strajnic, J" uniqKey="Strajnic J" first="J." last="Strajnic">J. Strajnic</name>
<name sortKey="Strajnic, J" sort="Strajnic, J" uniqKey="Strajnic J" first="J." last="Strajnic">J. Strajnic</name>
<name sortKey="Vachier, F" sort="Vachier, F" uniqKey="Vachier F" first="F." last="Vachier">F. Vachier</name>
</country>
<country name="Australie"><noRegion><name sortKey="Laas Bourez, M" sort="Laas Bourez, M" uniqKey="Laas Bourez M" first="M." last="Laas-Bourez">M. Laas-Bourez</name>
</noRegion>
</country>
</tree>
</affiliations>
</record>
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