Long GRB Jet Breaks

Details Long GRB Jet Breaks Long GRB Jet Breaks

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008cxo..prop.2723g&link_type=abstract

Chandra proposal ID #10500078

Computer Science

Scientific paper

In the standard fireball model for GRB afterglows, the jet opening angle can be determined from the achromatic jet break time by measuring the light curve until this break occurs. Swift XRT observations have shown that jet breaks are not observed in the first several days or weeks of a typical X-ray afterglow. This has important implications for the derived energetics of the GRB itself that cannot be resolved without a more complete sample of observed jet breaks. We propose to follow 4 carefully chosen long GRB afterglows with late-time Chandra observations in order to search for jet breaks occurring after the Swift observations end.

Affiliated with

Also associated with

No associations

Rating

Long GRB Jet Breaks 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 Long GRB Jet Breaks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long GRB Jet Breaks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1436058