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arxiv: astro-ph/0002207 · v1 · submitted 2000-02-09 · 🌌 astro-ph

Time Resolved GRB Spectroscopy

classification 🌌 astro-ph
keywords grbsinitialmodelopticallyotssmspectrathintime-resolved
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We present the main results of a study of time-resolved spectra of 43 intense GRBs detected by BATSE. We considered the 4-parameter Band model and the Optically Thin Synchrotron Shock model (OTSSM). We find that the large majority of time-resolved spectra of GRBs are in remarkable agreement with the OTSSM. However, about 15 % of initial GRB pulses show an apparent low-energy photon suppression. This phenomenon indicates that complex radiative conditions modifying optically thin emission may occur during the initial phases of some GRBs.

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