Multifrequency studies of Gamma-Ray bursts: towards the understanding of the mystery

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Invited review to be published in "Multifrequency studies of high energy sources", Eds.: Giovanelli, F. and Sabau-Graziati, L.

Scientific paper

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 GRBs 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 of the first optical/IR/radio counterparts in 1997-99, greatly improving our understanding of these sources. Now it is widely accepted that GRBs originate at cosmological distances. 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 or the merging of compact objects.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Multifrequency studies of Gamma-Ray bursts: towards the understanding of the mystery does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multifrequency studies of Gamma-Ray bursts: towards the understanding of the mystery, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multifrequency studies of Gamma-Ray bursts: towards the understanding of the mystery will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-573191

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.