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A&A 401, 129-140 (2003)
DOI: 10.1051/0004-6361:20021863
On the difference between the short and long gamma-ray bursts
L. G. Balázs1, Z. Bagoly2, I. Horváth3, A. Mészáros4 and P. Mészáros51 Konkoly Observatory, Budapest, Box 67, 1525, Hungary
2 Laboratory for Information Technology, Eötvös University, Budapest, Pázmány Péter sétány 1/A, 1117, Hungary
e-mail: bagoly@ludens.elte.hu
3 Dept. of Physics, Bolyai Military University, Budapest, Box 12, 1456, Hungary
e-mail: hoi@bjkmf.hu
4 Astronomical Institute of the Charles University, 180 00 Prague 8, V Holesovickách 2, Czech Republic
e-mail: meszaros@mbox.cesnet.cz
5 Dept. of Astronomy & Astrophysics, Pennsylvania State University, 525 Davey Lab
e-mail: nnp@astro.psu.edu
(Received 29 August 2002 / Accepted 16 December 2002)
Abstract
We argue that the distributions of both the intrinsic
fluence and the intrinsic duration of the
-ray emission in
gamma-ray bursts from the BATSE sample are well represented by
log-normal distributions, in which the intrinsic dispersion is
much larger than the cosmological time dilatation and redshift
effects. We perform separate bivariate log-normal distribution
fits to the BATSE short and long burst samples. The bivariate
log-normal behaviour results in an ellipsoidal distribution, whose
major axis determines an overall statistical relation between the
fluence and the duration. We show that this fit provides evidence
for a power-law dependence between the fluence and the duration,
with a statistically significant different index for the long and
short groups. We discuss possible biases, which might affect this
result, and argue that the effect is probably real. This may
provide a potentially useful constraint for models of long and
short bursts.
Key words: gamma-rays: bursts -- methods: statistical -- methods: data analysis
Offprint request: L. G. Balázs, balazs@konkoly.hu
© ESO 2003
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