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Evidences for two Gamma-Ray Burst afterglow emission regimes

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arxiv astro-ph/0008385 v1 pith:L55EWN6D submitted 2000-08-24 astro-ph

Michel Boer , Bruce Gendre This is my paper · ORCID
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keywords afterglowabsorptionburstcorrelationgamma-raygrbsmodeloptical
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We applied cosmological and absorption corrections to the X-ray and optical afterglow fluxes of a sample of Gamma-Ray Burst sources of known distance. We find a good correlation in X-rays and that the GRBs in our sample form two well defined classes. We tentatively interpret them as radiative and adiabatic afterglow behaviours in the framework of the fireball model for GRBs. We do not observe this correlation at optical wavelengths. This discrepancy with the model may be due to the absorption in the source vicinity.

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Cited by 1 Pith paper

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  1. A review of long lasting activities of the central engine of gamma-ray bursts

    astro-ph.HE 2025-01 unverdicted novelty 1.0 of 10

    A review of ultra-long gamma-ray bursts and X-ray plateau phases as evidence that the central engine keeps working long after the first flash.

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