Short gamma-ray bursts (GRBs), typically lasting less than 2 s, are a special class of GRBs of great interest. We report the detection by the AGILE satellite of the short GRB 090510 which shows two clearly distinct emission phases: a prompt phase lasting similar to 200 ms and a second phase lasting tens of seconds. The prompt phase is relatively intense in the 0.3-10 MeV range with a spectrum characterized by a large peak/cutoff energy near 3 MeV; in this phase, no significant high-energy gamma-ray emission is detected. At the end of the prompt phase, intense gamma-ray emission above 30 MeV is detected showing a power-law time decay of the flux of the type t(-1.3) and a broadband spectrum remarkably different from that of the prompt phase. It extends from sub-MeV to hundreds of MeV energies with a photon index alpha similar or equal to 1.5. GRB 090510 provides the first case of a short GRB with delayed gamma-ray emission. We present the timing and spectral data of GRB 090510 and briefly discuss its remarkable properties within the current models of gamma-ray emission of short GRBs.

Agile Detection Of Delayed Gamma-Ray Emission From The Short Gamma-Ray Burst Grb 090510

FERRARI, Attilio;
2010-01-01

Abstract

Short gamma-ray bursts (GRBs), typically lasting less than 2 s, are a special class of GRBs of great interest. We report the detection by the AGILE satellite of the short GRB 090510 which shows two clearly distinct emission phases: a prompt phase lasting similar to 200 ms and a second phase lasting tens of seconds. The prompt phase is relatively intense in the 0.3-10 MeV range with a spectrum characterized by a large peak/cutoff energy near 3 MeV; in this phase, no significant high-energy gamma-ray emission is detected. At the end of the prompt phase, intense gamma-ray emission above 30 MeV is detected showing a power-law time decay of the flux of the type t(-1.3) and a broadband spectrum remarkably different from that of the prompt phase. It extends from sub-MeV to hundreds of MeV energies with a photon index alpha similar or equal to 1.5. GRB 090510 provides the first case of a short GRB with delayed gamma-ray emission. We present the timing and spectral data of GRB 090510 and briefly discuss its remarkable properties within the current models of gamma-ray emission of short GRBs.
2010
708
L84
L88
A. Giuliani;F. Fuschino;G. Vianello;M. Marisaldi;S. Mereghetti;M. Tavani;S. Cutini;G. Barbiellini;F. Longo;E. Moretti;M. Feroci;E. D. Monte;A. Argan;A. Bulgarelli;P. Caraveo;P. W. Cattaneo;A. W. Chen;T. Contessi;F. D'Ammando;E. Costa;G. D. Paris;G. D. Cocco;I. Donnarumma;Y. Evangelista;A. Ferrari;M. Fiorini;M. Galli;F. Gianotti;C. Labanti;I. Lapshov;F. Lazzarotto;P. Lipari;A. Morselli;L. Pacciani;A. Pellizzoni;F. Perotti;G. Piano;P. Picozza;M. Pilia;G. Pucella;M. Prest;M. Rapisarda;A. Rappoldi;A. Rubini;S. Sabatini;E. Scalise;E. Striani;P. Soffitta;M. Trifoglio;A. Trois;E. Vallazza;S. Vercellone;V. Vittorini;A. Zambra;D. Zanello;C. Pittori;F. Verrecchia;P. Santolamazza;P. Giommi;S. Colafrancesco;L. A. Antonelli;L. Salotti
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/86345
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