Other
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1279..287b&link_type=abstract
DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS. AIP Conference Proceedings, Volume 1279, pp. 287-289 (2010).
Other
Gamma-Ray Sources (Astronomical), Astronomical Telescopes, Spectral Analysis, Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification
Scientific paper
We present one of the most intriguing results obtained with an updated catalog of 113 early time (i.e. tpk<~1000 s) and 36 late time (i.e. tpk>~1000 s) X-ray flares detected by Swift in the afterglows of Gamma-Ray Bursts (GRB): the evolution of the width of the flares with time. This result, together with other properties investigated on early and late time flares and bright flares, provides a clear observational property that every model aiming at explaining the GRB emission has to face.
Chincarini Guido
Grazia Bernardini Maria
Margutti Raffaella
No associations
LandOfFree
The evolution of the width of X-ray flares with time in Gamma-ray bursts 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 evolution of the width of X-ray flares with time in Gamma-ray bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution of the width of X-ray flares with time in Gamma-ray bursts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1403188