X-Ray Flares In GRB090812 - Case Study
Shlomo Dado, Arnon Dar
TL;DR
This paper demonstrates that the cannonball (CB) model accurately reproduces the light curves and spectral evolution of X-ray and optical flares in GRB090812, supporting its applicability to long-duration gamma-ray bursts.
Contribution
The study extends the CB model to successfully explain the X-ray and optical flares observed in GRB090812, highlighting its comprehensive predictive power.
Findings
CB model reproduces GRB090812 flare light curves
Spectral evolution matches observational data
Supports CB model as a unified explanation for GRB emissions
Abstract
The master formulae of the CB model of long durations gamma ray bursts (GRBs) which reproduce very well the light curves and spectral evolution of their prompt emission pulses and their smooth afterglows, also reproduce very well the lightcurves and spectral evolution of their X-ray and optical flares. Here we demonstrate that for GRB090812
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astro and Planetary Science · Astronomy and Astrophysical Research