Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-01-07
Astronomy and Astrophysics
Astrophysics
Replaces previous version: now it does include figure. Accepted for publication in the Astrophysical Journal Letters
Scientific paper
10.1086/310542
I consider the recent discovery of a soft X-ray source inside the error box of the gamma ray burst GB 960720 by the SAX, ASCA and ROSAT satellites, in terms of the fireball model. I show that the ejecta shell, which, after causing the burst is cold and dense, but still relativistic, keeps plowing through the interstellar medium, heating up the just-shocked matter which then emits X-rays. I compute the radiation emitted by this matter. I show that, up to about two months after the burst, in the cosmological scenario a soft X-ray (0.1-10 keV) flux of at least 10^(-13) erg / s cm^2, well within current observational capabilities, is generated, explaining the observations of the three satellites. Instead, in the Galactic Halo scenario a flux 3 orders of magnitude lower is expected. Detection of this non-thermal, declining flux in a statistically significant number of objects would simultaneously establish the fireball model and the cosmological nature of gamma ray bursts.
No associations
LandOfFree
The soft X-ray afterglow of gamma ray bursts, a stringent test for the fireball model 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 The soft X-ray afterglow of gamma ray bursts, a stringent test for the fireball model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The soft X-ray afterglow of gamma ray bursts, a stringent test for the fireball model will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-387693