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2007MNRAS.374.1473B - Mon. Not. R. Astron. Soc., 374, 1473-1478 (2007/February-1)
The Swift gamma-ray burst GRB 050422.
BEARDMORE A.P., PAGE K.L., O'BRIEN P.T., OSBORNE J.P., KOBAYASHI S., ZHANG B., BURROWS D.N., CAPALBI M., GOAD M.R., GODET O., HILL J.E., LA PAROLA V., MARSHALL F. and WELLS A.A.
Abstract (from CDS):
In comparison with other Swift bursts, GRB050422 was unusually X-ray faint, had a soft X-ray spectrum, and had an unusually steep early X-ray decline. Even so, its behaviour can be accommodated by standard models. The combined BAT/XRT light curve indicates that the initial, steeply declining, X-ray emission is related to the tail of the prompt gamma-ray emission. The shallower decay seen after the break is consistent with the standard afterglow model.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): gamma-rays: bursts
Simbad objects: 12
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