What did we learn from the extremely bright gamma ray bursts 990123 and 080319B?

Details What did we learn from the extremely bright gamma ray bursts 990123 and 080319B? What did we learn from the extremely bright gamma ray bursts 990123 and 080319B?

2008-12-17

arxiv.org/abs/0812.3340v2

Astronomy and Astrophysics

Astrophysics

Added references. Corrected label in Fig. 7

Scientific paper

The two brightest and so far the best studied gamma ray bursts (GRBs), 990123 and 080319B, were ordinary, highly collimated GRBs produced in a core collapse supernova explosion within a high-density wind environment and observed from a very near-axis viewing angle. Inverse Compton scattering (ICS) and synchrotron radiation (SR), the two dominant radiation mechanisms in the cannonball (CB) model of GRBs, together with the burst environment, provide a very simple and sufficiently accurate description of the multiwavelength lightcurves of their prompt and afterglow emissions.

Affiliated with

Also associated with

No associations

Rating

What did we learn from the extremely bright gamma ray bursts 990123 and 080319B? 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 What did we learn from the extremely bright gamma ray bursts 990123 and 080319B?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and What did we learn from the extremely bright gamma ray bursts 990123 and 080319B? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-95602