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The spectral sharpness angle of gamma-ray bursts

We explain the results of Yu et al. (2015b) of the novel sharpness angle measurement to a large number of spectra obtained from the Fermi gamma-ray burst monitor. The sharpness angle is compared to the values obtained from...
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Applying an accurate spherical model to gamma-ray burst afterglow observations
We present results of model fits to afterglow data sets of GRB 970508, GRB 980703 and GRB 070125, characterized by long and broad-band coverage. The model assumes synchrotron radiation (including self-absorption) from a...
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Self-similar relativistic blast waves with energy injection
Hendrik Van Eerten
Aug 21, 2014
A sufficiently powerful astrophysical source with power-law luminosity in time will give rise to a self-similar relativistic blast wave with a reverse shock travelling into the ejecta and a forward shock moving into the...
Published by:
Applying an accurate spherical model to gamma-ray burst afterglow observations
We present results of model fits to afterglow data sets of GRB 970508, GRB 980703 and GRB 070125, characterized by long and broad-band coverage. The model assumes synchrotron radiation (including self-absorption) from a...
Published by:
Jet simulations and gamma-ray burst afterglow jet breaks
he conventional derivation of the gamma-ray burst afterglow jet break time uses only the blast wave fluid Lorentz factor and therefore leads to an achromatic break. We show that in general gamma-ray burst afterglow jet breaks...
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The sharpness of gamma-ray burst prompt emission spectra
Context. We study the sharpness of the time-resolved prompt emission spectra of gamma-ray bursts (GRBs) observed by the Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope.

Aims. We aim to obtain...
Published by:
The spectral sharpness angle of gamma-ray bursts

We explain the results of Yu et al. (2015b) of the novel sharpness angle measurement to a large number of spectra obtained from the Fermi gamma-ray burst monitor. The sharpness angle is compared to the values obtained from...
Published by:
Self-similar relativistic blast waves with energy injection
Hendrik Van Eerten
Aug 21, 2014
A sufficiently powerful astrophysical source with power-law luminosity in time will give rise to a self-similar relativistic blast wave with a reverse shock travelling into the ejecta and a forward shock moving into the...
Published by:
Jet simulations and gamma-ray burst afterglow jet breaks
he conventional derivation of the gamma-ray burst afterglow jet break time uses only the blast wave fluid Lorentz factor and therefore leads to an achromatic break. We show that in general gamma-ray burst afterglow jet breaks...
Published by:
The sharpness of gamma-ray burst prompt emission spectra
Context. We study the sharpness of the time-resolved prompt emission spectra of gamma-ray bursts (GRBs) observed by the Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope.

Aims. We aim to obtain...
Published by: