Results 31 to 40 of about 58,014 (248)
The Astrophysical Journal Letters, 2023 GRB 230307A is one of the brightest gamma-ray bursts detected so far. With the excellent observation of GRB 230307A by the Fermi Gamma-ray Burst Monitor, we can reveal the details of prompt emission evolution.
Yun Wang +4 more
doaj +1 more source
GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst
The Astrophysical Journal Letters, 2023 We report the discovery of the unusually bright long-duration gamma-ray burst (GRB), GRB 221009A, as observed by the Neil Gehrels Swift Observatory (Swift), Monitor of All-sky X-ray Image, and Neutron Star Interior Composition Explorer Mission.
Maia A. Williams +55 more
doaj +1 more source
Compton Dragged Gamma--Ray Bursts associated with Supernovae [PDF]
, 1999 It is proposed that the gamma-ray photons that characterize the prompt emission of Gamma-Ray Bursts are produced through the Compton drag process, caused by the interaction of a relativistic fireball with a very dense soft photon bath.
Annalisa Celotti +5 more
core +2 more sources
CLOAKED GAMMA-RAY BURSTS [PDF]
The Astrophysical Journal, 2014 accepted for publication in the Astrophysical ...
openaire +2 more sources
Model Constraints Based on the IceCube Neutrino Nondetection of GRB 221009A
The Astrophysical Journal, 2023 GRB 221009A is a bright gamma-ray burst (GRB) with isotropic energy larger than 10 ^54 erg. Its fairly low redshift makes it a promising candidate for high-energy neutrino detection.
Shunke Ai, He Gao
doaj +1 more source
On the nature of gamma-ray burst time dilations [PDF]
, 1994 The recent discovery that faint gamma-ray bursts are stretched in time relative to bright ones has been interpreted as support for cosmological distances: faint bursts have their durations redshifted relative to bright ones.
Paczyński, Bohdan +1 more
core +3 more sources
Gamma-Ray Burst Energetics [PDF]
The Astrophysical Journal, 1999 We estimate the fraction of the total energy in a Gamma-Ray Burst (GRB) that is radiated in photons during the main burst. Random internal collisions among different shells limit the efficiency for converting bulk kinetic energy to photons. About 1% of the energy of explosion is converted to radiation, in 10-1000 kev energy band in the observer frame ...
openaire +2 more sources
Repeating Emission Episodes in Gamma-Ray Bursts: Millilensing or Jet Precession?
The Astrophysical Journal, 2023 Recently, some gamma-ray bursts (GRBs) whose light curves consist of repeating emission episodes with similar temporal profiles have attracted extensive attention.
He Gao +3 more
doaj +1 more source
Are There MeV Gamma-Ray Bursts? [PDF]
, 1995 It is often stated that gamma-ray bursts (GRBs) have typical energies of several hundred keV. Is this a real feature of GRBs or is it due to an observational bias?
Narayan, Ramesh, Piran, Tsvi
core +3 more sources
The design of a gamma‐ray burst polarimeter [PDF]
, 1993 The study of the polarization properties of the gamma‐ray bursts is the one remaining unexplored avenue of research which may help to answer some of the fundamental problems regarding the nature of these mysterious objects. We have designed an instrument
Forrest, D J +3 more
core +2 more sources