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

A. Giuliani
•
F. Fuschino
•
G. Vianello
altro
L. Salotti
2010
  • journal article

Periodico
THE ASTROPHYSICAL JOURNAL LETTERS
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.
DOI
10.1088/2041-8205/708/2/L84
WOS
WOS:000273308000004
Archivio
http://hdl.handle.net/11368/2338219
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-77949564308
Diritti
metadata only access
Soggetti
  • High Energy Gamma-ray...

  • AGILE satellite

  • Gamma-ray Bursts

Web of Science© citazioni
45
Data di acquisizione
Mar 20, 2024
Visualizzazioni
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Data di acquisizione
Apr 19, 2024
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