The origin of X-ray flash observed by HETE-2

Details The origin of X-ray flash observed by HETE-2 The origin of X-ray flash observed by HETE-2

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..507s&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 8, p. 507 - 517 (2005)

Astronomy and Astrophysics

Astronomy

1

X-Ray Bursts

Scientific paper

We present the detailed and systematic study of the spectral characteristics of X-ray flashes (XRFs) observed by HETE-2. The XRFs show similar characteristics to the long GRBs except for their lower Epeak energies. One of the key observational relation, Epeak-Eiso relation, is discussed as a frame work to understand the gamma-ray burst in an unified picture. We emphasis on the importance of the partnership between HETE and Swift for solving the nature of XRFs.

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