Observations and theoretical models of gamma-ray bursts

Abstract

GRBs have remained a puzzle for many high-energy astrophysicists since their discovery in 1967. With the advent of the X-ray satellites BeppoSAX and RossiXTE, it has been possible to carry out deep multi-wavelength observations of the counterparts associated with the long GRBs class just within a few hours of occurence, thanks to the observation of the fading X-ray emission that follows the more energetic gamma-ray photons once the GRB event has ended. The fact that this emission (the afterglow) extends at longer wavelengths, has led to the discovery optical/IR/radio counterparts in 1997-2000, greatly improving our understanding of these sources. Now it is widely accepted that GRBs originate at cosmological distances with energie releases of 10^51-10^53 ergs. About 25 host galaxies have been detected so far for long-duration GRBs. The observed afterglow satisfies the predictions of the "standard" relativistic fireball model, and the central engines that power these extraordinary events are thought to be the collapse of massive stars rather than the merging of compact objects as previously also suggested. Short GRBs still remain a mystery as no counterparts have been detected.