Fermi detection of delayed GeV emission from the short gamma-ray burst 081024B
Abstract
Here, we report on the detailed analysis of the high-energy extended emission from the short gamma-ray burst (GRB) 081024B detected by the Fermi Gamma-ray Space Telescope. Historically, this represents the first clear detection of temporal extended emission from a short GRB. Furthermore, the light curve observed by the Fermi Gamma-ray Burst Monitor lasts approximately 0.8 s whereas the emission in the Fermi Large Area Telescope lasts for about 3 s. Evidence of longer lasting high-energy emission associated with long bursts has been already reported by previous experiments. These observations, together with the earlier reported study of the bright short GRB 090510, indicate similarities in the high-energy emission of short and long GRBs and open the path to new interpretations.
- Authors:
-
- Naval Research Lab. (NRL), Washington, DC (United States); National Academy of Sciences, Washington, DC (United States); et al.
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- Contributing Org.:
- Fermi LAT Collaboration
- OSTI Identifier:
- 1357573
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 712; Journal Issue: 1; Journal ID: ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; gamma-ray burst: general; gamma-ray burst: individual (GRB 081024B)
Citation Formats
Abdo, A. A. Fermi detection of delayed GeV emission from the short gamma-ray burst 081024B. United States: N. p., 2010.
Web. doi:10.1088/0004-637X/712/1/558.
Abdo, A. A. Fermi detection of delayed GeV emission from the short gamma-ray burst 081024B. United States. https://doi.org/10.1088/0004-637X/712/1/558
Abdo, A. A. Wed .
"Fermi detection of delayed GeV emission from the short gamma-ray burst 081024B". United States. https://doi.org/10.1088/0004-637X/712/1/558. https://www.osti.gov/servlets/purl/1357573.
@article{osti_1357573,
title = {Fermi detection of delayed GeV emission from the short gamma-ray burst 081024B},
author = {Abdo, A. A.},
abstractNote = {Here, we report on the detailed analysis of the high-energy extended emission from the short gamma-ray burst (GRB) 081024B detected by the Fermi Gamma-ray Space Telescope. Historically, this represents the first clear detection of temporal extended emission from a short GRB. Furthermore, the light curve observed by the Fermi Gamma-ray Burst Monitor lasts approximately 0.8 s whereas the emission in the Fermi Large Area Telescope lasts for about 3 s. Evidence of longer lasting high-energy emission associated with long bursts has been already reported by previous experiments. These observations, together with the earlier reported study of the bright short GRB 090510, indicate similarities in the high-energy emission of short and long GRBs and open the path to new interpretations.},
doi = {10.1088/0004-637X/712/1/558},
journal = {The Astrophysical Journal},
number = 1,
volume = 712,
place = {United States},
year = {2010},
month = {3}
}
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