Astronomy and Astrophysics – Astrophysics
Scientific paper
2002-11-07
Astronomy and Astrophysics
Astrophysics
11 pages, 1 figure
Scientific paper
We present the main observational features expected for GRBs that occur inside pulsar wind bubbles (PWBs). This is the most natural outcome of supranova model where initially a supernova explosion takes place, leaving a supra-massive NS, which loses its rotational energy over a time t_sd and collapses to a BH, triggering a GRB explosion. We find that the time delay t_sd between the supernova and GRB events is the most important parameter that determines the behavior of the system. We consider the afterglow, prompt GRB and direct emission from the PWB. The observational signatures for different t_sd are described and joined together into one coherent framework. Constraints on the model are derived for a spherical PWB, from the lack of detection of the PWB emission and afterglow observations. For very low values of t_sd<1 hr the supranova model reduces to the collapsar model; 0.4
Granot Jonathan
Guetta Dafne
No associations
LandOfFree
Gamma-Ray Bursts in Pulsar Wind Bubbles: Putting the Pieces Together 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 Gamma-Ray Bursts in Pulsar Wind Bubbles: Putting the Pieces Together, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-Ray Bursts in Pulsar Wind Bubbles: Putting the Pieces Together will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-406771