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  5. AGILE and Konus-Wind Observations of GRB 190114C: The Remarkable Prompt and Early Afterglow Phases
 

AGILE and Konus-Wind Observations of GRB 190114C: The Remarkable Prompt and Early Afterglow Phases

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2020
Author(s)
URSI, ALESSANDRO  
•
TAVANI, MARCO  
•
Frederiks, D. D.
•
Romani, M.
•
VERRECCHIA, Francesco  
•
MARISALDI, MARTINO  
•
Aptekar, R. L.
•
ANTONELLI, Lucio Angelo  
•
ARGAN, ANDREA  
•
BULGARELLI, ANDREA  
•
Barbiellini, G.
•
CARAVEO, PATRIZIA  
•
CARDILLO , MARTINA  
•
CASENTINI, CLAUDIO  
•
Cattaneo, P. W.
•
Chen, A.
•
COSTA, ELIA  
•
Donnarumma, I.
•
EVANGELISTA, YURI  
•
FEROCI, MARCO  
•
Ferrari, A.
•
FUSCHINO, FABIO  
•
Galli, M.
•
GIULIANI, ANDREA  
•
LABANTI, CLAUDIO  
•
LAZZAROTTO, FRANCESCO  
•
Longo, F.
•
LUCARELLI, Fabrizio  
•
Morselli, A.
•
Paoletti, F.
•
PARMIGGIANI, NICOLO  
•
PIANO, Giovanni  
•
PILIA, Maura  
•
PITTORI, Carlotta  
•
Svinkin, D. S.
•
TROIS, ALESSIO  
•
Tsvetkova, A. E.
•
VERCELLONE, STEFANO  
•
VITTORINI, VALERIO  
DOI
10.3847/1538-4357/abc2d4
Abstract
GRB 190114C represents a breakthrough for the physics of gamma-ray bursts (GRBs), being the first GRB with delayed emission above 300 GeV, as reported by MAGIC. We present in this paper the sub-MeV/MeV data of the prompt and early afterglow emissions of GRB 190114C, as detected by AGILE and Konus-Wind, in the 20 keV-100 MeV energy range. The first stages of the burst exhibit multiple emission components, associated with an interesting spectral evolution. The first 2 s of the prompt emission can be described by a single "Band-like" spectral component. The successive 4 s show the presence of an additional high-energy spectral component, which quickly evolves into a "hard-flat" component of the νFν spectrum, extending up to 10-100 MeV and likely produced by inverse Compton radiation, whose onset and evolution are clearly shown in our data. After this phase, the νFν spectrum evolves into a "V shape," showing the persistence and spectral hardening of the additional high-energy component in substantial agreement with Fermi and Swift results. We also analyze the first ∼200 s of the early afterglow that show a reflaring episode near T0 + 15 s. We identify a new, so-far-unnoticed flux temporal break near T0 + 100 s, which is detected in hard X-rays by both Konus-Wind and INTEGRAL/SPI-ACS. We find this break incompatible with the commonly assumed adiabatic evolution of a fireball in a constant-density medium. We interpret this break as a consequence of radiative evolution of the early afterglow from a fireball expanding in a wind-like circumburst medium.
Volume
904
Issue
2
Start page
133
Uri
http://hdl.handle.net/20.500.12386/31936
Url
https://doi.org/10.3847/1538-4357/abc2d4
https://iopscience.iop.org/article/10.3847/1538-4357/abc2d4
Issn Identifier
0004-637X
Ads BibCode
2020ApJ...904..133U
Rights
restricted
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Ursi_2020_ApJ.pdf

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282a49e714222189695ac61cf3ce853b

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