Gamma-Ray Burst Progenitors: Probing Their Environment

Astronomy and Astrophysics – Astronomy

Scientific paper

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Chandra Proposal Id #03500014

Scientific paper

Gamma-ray burst astronomy is a field maturing at a phenomenal rate. Only three years after the discovery of fading long-wavelength counterparts, we now have distance measurements for dozens of events, we have developed a detailed theoretical framework for understanding the X-ray -- radio afterglow lightcurves, and observational evidence now ties the progenitors of long GRBs (those studied to-date) to the collapse of massive stars. While progress has been rapid, three important new observational and theoretical discoveries, formulated over the last twelve months, allow us to address new and in many cases more sophisticated questions than could have been posed a year ago.

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