Short Gamma-Ray Bursts Observed by PHEBUS

Details Short Gamma-Ray Bursts Observed by PHEBUS Short Gamma-Ray Bursts Observed by PHEBUS

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.231..115d&link_type=abstract

Astrophysics and Space Science, Volume 231, Issue 1-2, pp. 115-118

Astronomy and Astrophysics

Astrophysics

3

Gamma-Ray Bursts

Scientific paper

Statistical studies of Gamma-Ray Burst (GRB) properties have recently led to the discovery of a subclass within the population of classical events (Dezalayet al. 1992, Kouveliotouet al. 1993). Bursts belonging to this subclass are characterized by short durations, typically less than 2 seconds, and harder spectra on average. Using the PHEBUS GRB data set, we analyse the distributions of peak intensity, hardness ratio, and duration of the two subclasses. We also compare the sum spectra obtained with the brightest events to determine the ratio of total energies observed for each population.

Affiliated with

Also associated with

No associations

Rating

Short Gamma-Ray Bursts Observed by PHEBUS 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 Short Gamma-Ray Bursts Observed by PHEBUS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Short Gamma-Ray Bursts Observed by PHEBUS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-823406