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A&A 379, L39-L43 (2001)
DOI: 10.1051/0004-6361:20011485
Possible detection of hard X-ray afterglows of short
-ray bursts
D. Lazzati1, E. Ramirez-Ruiz1 and G. Ghisellini2
1 Institute of Astronomy, University of Cambridge, Madingley Road, CB3 0HA Cambridge, UK
e-mail: enrico@ast.cam.ac.uk
2 Osservatorio Astronomico di Brera, via Bianchi 46, 23807 Merate, Italy
e-mail: gabriele@merate.mi.astro.it
(Received 31 August 2001 / Accepted 10 October 2001 )
Abstract
We report the discovery of a transient and fading hard X-ray emission
in the BATSE lightcurves of a sample of short
-ray bursts. We
have summed each of the four channel BATSE light curves of 76 short
bursts to uncover the average overall temporal and spectral evolution
of a possible transient signal following the prompt flux. We found an
excess emission peaking ~30 s after the prompt one, detectable
for
100 s. The soft power-law spectrum and the
time-evolution of this transient signal suggest that it is produced by
the deceleration of a relativistic expanding source, as predicted by
the afterglow model.
Key words: gamma rays: bursts -- radiation mechanisms: non-thermal
Offprint request: D. Lazzati, lazzati@ast.cam.ac.uk
SIMBAD Objects
© ESO 2001
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