Decomposition of a cosmic gamma-ray burst into two non-correlated radiation components

Details Decomposition of a cosmic gamma-ray burst into two non-correlated radiation components Decomposition of a cosmic gamma-ray burst into two non-correlated radiation components

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.274..361c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 274, Issue 2, pp. 361-368.

Astronomy and Astrophysics

Astronomy

5

Gamma-Rays: Bursts

Scientific paper

The emission of gamma-ray burst GB 881024 is decomposed into two physically distinct non-correlated components by means of a technique called rate-rate diagrams. One of the components dominates at energies below 250 keV and the other one dominates above 250 keV. Time histories and rate/spectrum evolution of the components are considered. The low-energy component manifests clear hardness/rate correlation while the high-energy one does not. The main known types of hardness/rate evolution of gamma-ray bursts are then explained as a result of superposition of components. Possible astrophysical consequences are discussed.

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