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Spectral Evolution of Short GRBS on sub-millisecond timescale

Published online by Cambridge University Press:  22 July 2013

A. Chernenko*
Affiliation:
Space Research Institute, Moscow
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Abstract

There has been growing consensus that short and long GRBs are associated with twodifferent populations of astrophysical sources: mergers and SN explosions, respectively.While temporal properties of short and long GRBs could be considered with similar depthand accuracy, patterns of spectral variability of the 2 classes of GRBs are much harder tocompare. This is due to the fact, that short GRBs exhibit variability on time scalesshorter than 1 ms and count rate, measured at such short time scales, is not sufficientfor reliable spectroscopy even for the brightest events.

In this situation, any new possibility to look at spectral evolution of short GRBs onsub-millisecond time scales in terms of spectral parameters, may provide more solidbackground for theoretical analysis. In this paper we present analysis of spectralevolution of short GRBs in terms of Band spectral function parameters, using the earlierdeveloped Global Fit approach (GFA).

Type
Research Article
Copyright
© EAS, EDP Sciences 2013

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References

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Chernenko, A., 2002, in the Proceedings of the IAU 8th Asian-Pacific Regional meeting, v.2, ed. S. Ikeuchi, J. Hearnshaw & T. Hanawa, 321