Generic signatures of the time profiles of BATSE cosmic gamma-ray bursts

Citation
Ig. Mitrofanov et al., Generic signatures of the time profiles of BATSE cosmic gamma-ray bursts, ASTROPHYS J, 504(2), 1998, pp. 925-934
Citations number
13
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
504
Issue
2
Year of publication
1998
Part
1
Pages
925 - 934
Database
ISI
SICI code
0004-637X(19980910)504:2<925:GSOTTP>2.0.ZU;2-I
Abstract
A new method is proposed, which allows the study of generic signatures of c osmic gamma-ray burst time histories. We average the 64 ms resolution time profiles of 275 bright bursts detected by BATSE. The profile of each burst is normalized by the maximum number of counts at the peak of the primary pu lse, and individual pulses and interpulse valleys are selected from the nor malized pro files by identical selection criteria. New generic temporal par ameters are introduced, which characterize the duration and equivalent widt h of each pulse and the duration of each valley. The histograms of the tota l equivalent pulse width and summed pulse duration are bimodal. Bimodality is also seen in the histogram of the mean duration of individual pulses. Bu rsts from the short and long peaks of these distributions correspond to the two modes of the Third BATSE Burst Catalog T-50 and T-90 distributions. Th erefore, these new burst parameters demonstrate that the observed bimodal t emporal behavior results from properties of the pulsed emission of gamma-ra y bursts. The long mode of the T-90 histogram includes bursts with from one to similar to 20 pulses; the logarithmic mean pulse duration is 1.17 +/- 0 .09 s; for the long events with more than one pulse, the logarithmic mean v alley duration is 1.28 +/- 0.15 s. Bursts of the short mode of T-90 are mai nly single-pulse events, and the logarithmic mean pulse duration is much sm aller, 0.20 +/- 0.01 s. For multipulse bursts of the T-90 long mode, margin al correlations were found between the parameters of the pulses and valleys and the number of pulses. The basic signatures of the evolution of pulses and valleys along the time course of bursts are examined. Conclusions are d rawn concerning the physics of gamma-ray emission by taking into account th ese signatures.