Titlebook: Gamma-Ray Bursts in the Afterglow Era; Proceedings of the I Enrico Costa,Filippo Frontera,Jens Hjorth Conference proceedings 2001 Springer-

一再困擾

aerial

散步

能量守恒

ATOPY

Deject

Filibuster

Grundlegende Matrizenoperationen, fact very soft, x-ray rich, untriggered gamma ray bursts, in which the peak energy in 2-10 keV x-rays could be up to a factor of 100 larger than the peak energy in the 50-300 keV gamma ray range. The frequency is . yr..

Suggestions

Peter Lugner,Werner Mack,Manfred Pl?chl detected in common with .SAX. Temporaland spectralc haracteristics, such as peak flux, fluence, duration, and spectrum are compared to the full population of triggered BATSE GRBs. We find that FXTs have softer spectra than most triggered bursts, but that they are consistent with the extrapolated hardness expected for low-intensity GRBs.

煩憂

K. Friehs,B. Hitzmann,T. Scheperignificantly distinct pulse peaks, we find an order of magnitude fewer pulses than found in studies of long bursts. The disparity in lag magnitude is discontinuous across the .-s valley between long and short bursts. Thus, short bursts do not appear to be representable as a continuation of long bursts’ temporalc haracteristics.

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