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Low frequency observations of the radio nebula produced by the giant flare from SGR 1806-20
H. Spreeuw, B. Scheers, R. A. M. J. Wijers
The 2004 December 27 giant flare from SGR 1806-20 produced a radio nebula that was detectable for weeks. It was observed at a wide range of radio frequencies. We made a total of 19…
No visible optical variability from a relativistic blast wave encountering a wind-termination shock
H. J. van Eerten, Z. Meliani, R. A. M. J. Wijers +1
Gamma-ray burst afterglow flares and rebrightenings of the optical and X-ray light curve have been attributed to both late time inner engine activity and density changes in the med…
From blast wave to observation
H. J. van Eerten, R. A. M. J. Wijers
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 t…