X-ray observations of afterglows are providing new insights on the nature of the central source of GRB. In this review I will focus on observations of temporal and spectral features, particularly on iron lines by BeppoSAX & Chandra and discuss how these observations can disclose the origin of the progenitors of GRB. I briefly review the old and new mysteries opened by recent observations and discuss observational prospects and future perspectives of GRB science.
CITATION STYLE
Piro, L. (2006). X-Ray Afterglows and Features of Gamma-Ray Bursts. In Gamma-Ray Bursts in the Afterglow Era (pp. 97–105). Springer-Verlag. https://doi.org/10.1007/10853853_26
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