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

A. Corsi, L. Piro

Research output: Contribution to journalArticlepeer-review

6 Scopus citations


Aims. We investigate for possible evidence of inverse Compton (IC) emission in the X-ray afterglow of XRF 050406. Methods. In the framework of the standard fireball model, we show how the late-time flattening observed in the X-ray light curve between ∼104 s and ∼106 s can be explained in a synchrotron-plus-IC scenario when the IC peak frequency crosses the X-ray band. Results. We thus conclude that the appearance of an IC component above the synchrotron one at late times successfully accounts for these X-ray observations.

Original languageEnglish
Pages (from-to)741-746
Number of pages6
JournalAstronomy and Astrophysics
Issue number3
StatePublished - Nov 2006


  • Gamma rays: bursts
  • Radiation mechanisms: non-thermal
  • X-rays: bursts
  • X-rays: individuals: XRF 050406


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