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arXiv · astro-ph/0604158

XRF 050406 late-time flattening: an inverse Compton component?

A. Corsi·L. Piro
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Abstract

We investigate for possible evidence of inverse Compton (IC) emission in the X-ray afterglow of XRF 050406. In the framework of the standard fireball model, we show how the late-time flattening observed in the X-ray light curve between \~10^{4} s and ~10^{6} s can be explained in a synchrotron-plus-IC scenario, when the IC peak frequency crosses the X-ray band. We thus conclude that the appearance of an IC component above the synchrotron one at late times successfully accounts for these X-ray observations.

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A. Corsi, L. Piro. 2007-01-08. XRF 050406 late-time flattening: an inverse Compton component?. https://doi.org/10.1051/0004-6361%3A20065280

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