Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-12-09
Astron.Astrophys. 399 (2003) 505-510
Astronomy and Astrophysics
Astrophysics
6 pages, 2 figures. Accepted for publication in Astronomy and Astrophysics
Scientific paper
10.1051/0004-6361:20021825
There are observational facts and theoretical arguments for an origin of gamma-ray bursts in molecular clouds in distant galaxies. If this is true, one could detect a significant flux of GRB prompt and early afterglow X-ray radiation scattered into our line of sight by the molecular and atomic matter located within tens of parsecs of the GRB site long after the afterglow has faded away. The scattered flux directly measures the typical density of the GRB ambient medium. Furthemore, if the primary emission is beamed, the scattered X-ray flux will be slowly decreasing for several months to years before falling off rapidly. Therefore, it should be possible to estimate the collimation angle of a burst from the light curve of its X-ray echo and a measured value of the line-of-sight absorption column depth. It is shown that detection of such an echo is for the brightest GRBs just within the reach of the Chandra and XMM-Newton observatories.
Sazonov Sergei
Sunyaev Rachid
No associations
LandOfFree
Observing scattered X-ray radiation from gamma-ray bursts: a way to measure their collimation angles 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 Observing scattered X-ray radiation from gamma-ray bursts: a way to measure their collimation angles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observing scattered X-ray radiation from gamma-ray bursts: a way to measure their collimation angles will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-488394