Results 11 to 20 of about 2,993 (188)
Gamma-ray burst detection prospects for next generation ground-based VHE facilities [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT Gamma-ray Bursts (GRB) were discovered by satellite-based detectors as powerful sources of transient γ-ray emission. The Fermi satellite detected an increasing number of these events with its dedicated Gamma-ray Burst Monitor (GBM), some of which were associated with high energy photons ($E \gt 10$ GeV), by the Large Area ...
La Mura G. +8 more
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A generic dynamical model of gamma-ray burst remnants [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 10 pages, LaTeX, 4 postscript figures, accepted for publication in ...
Huang, Y. F., Dai, Z. G., Lu, T.
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Generation of circular polarization of gamma ray bursts [PDF]
Physical Review D, 2016 The generation of the circular polarization of Gamma Ray Burst (GRB) photons is discussed in this paper via their interactions with astroparticles in the presence or absence of background fields such as magnetic fields and non-commutative space time geometry.
Batebi, S. +4 more
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Gamma-ray burst afterglow scaling coefficients for general density profiles [PDF]
Monthly Notices of the Royal Astronomical Society, 2009 Gamma-ray burst (GRB) afterglows are well described by synchrotron emission originating from the interaction between a relativistic blast wave and the external medium surrounding the GRB progenitor. We introduce a code to reconstruct spectra and light curves from arbitrary fluid configurations, making it especially suited to study the effects of fluid ...
van Eerten, H.J., Wijers, R.A.M.J.
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Possible geometries of afterglow generation in the gamma-ray burst GRB 990705 [PDF]
Astronomy & Astrophysics, 2003 5 pages, 1 figures, final version, Astronomy & Astrophysics, in ...
Wang, X. Y., Dai, Z. G., Lu, T.
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ARE LOW-LUMINOSITY GAMMA-RAY BURSTS GENERATED BY RELATIVISTIC JETS? [PDF]
The Astrophysical Journal, 2011 Low-luminosity gamma-ray bursts (ll-GRBs) constitute a subclass of GRBs that play a central role in the GRB-supernova connection. While ll-GRBs differ from typical long GRBs (LGRBs) in many aspects, they also share some common features. Therefore, the question whether the gamma-ray emission of ll-GRBs and LGRBs has a common origin is of great interest.
Omer Bromberg, Ehud Nakar, Tsvi Piran
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Gamma‐ray Burst Models: General Requirements and Predictions [PDF]
Annals of the New York Academy of Sciences, 1995 ABSTRACTWhatever the ultimate energy source of gamma‐ray bursts turns out to be, the resulting sequence of physical events is likely to lead to a fairly generic, almost unavoidable scenario: a relativistic fireball that dissipates its energy after it has become optically thin. This is expected both for cosmological and halo distances.
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A General Data Quality Inspection for Gamma-Ray Bursts Searches with HAWC [PDF]
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017), 2017 Presented at the 35th International Cosmic Ray Conference (ICRC2017), Bexco, Busan, Korea.
de León, Cederik +2 more
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Generation of Magnetic Fields in the Relativistic Shock of Gamma‐Ray Burst Sources [PDF]
The Astrophysical Journal, 1999 12 pages, 2 figures included.
Medvedev, Mikhail V., Loeb, Abraham
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A General Overview for Localizing Short Gamma-Ray Bursts with a CubeSat Mega-Constellation [PDF]
Frontiers in Astronomy and Space Sciences, 2020 The Gamma-Ray Burst Monitor (GBM) on the {\it Fermi Gamma-Ray Space Telescope}, for the first time, detected a short gamma ray burst (SGRB) signal that accompanies a gravitational wave signal GW170817 in 2017. The detection and localization of the gravitational wave and gamma-ray source led all other space- and ground-based observatories to measure its
Fadil Inceoglu +5 more
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