NASA NTRS · 19930014717
Spectral evolution during a complex gamma ray burst observed with BATSE
Abstract
More than 270 gamma ray bursts have been observed to date with the BATSE (Burst and Transient Source Experiment) aboard the Compton Gamma Ray Observatory. Many have a duration of 10 seconds or more and complex structure with multiple peaks or spikes. Complex bursts in the energy range 30 keV to 1 MeV were systematically analyzed to determine the relations between intensity and spectral shape, or hardness. The burst hardness rises and falls in during spikes, but somewhat earlier than the intensity. A simple correlation between intensity and hardness is, therefore, not observed: the intensity lags instead. Results from one burst which shows evidence for longer lags in longer spikes are reported.
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Gruber, D. E., Band, D. L., Ford, L., Matteson, J. L., Meegan, C. L., Wilson, R. B., Fishman, G. J., Paciesas, W. S., Pendleton, G. N., Schaefer, B.. 1992-07-01. Spectral evolution during a complex gamma ray burst observed with BATSE. https://ntrs.nasa.gov/citations/19930014717
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