TP-10
Using the numerical code (Moderski, Sikora, Bulik; 1999) we calculate the lightcurves of gamma-ray burst afterglows. We analyze the dependence on the initial Lorentz factor, the collimation angle , the location of the observer, and including the lateral outflow of the expanding shell. We discuss the results in the framework of recently observed gamma-ray bursts (GRB990123 and GRB990510).
Fifth Huntsville Gamma Ray Burst Symposium
Hunsville, Alabama, USA
18-22 October, 1999