The Study of the Early X-Ray Afterglows About Bright and Dark GRBs

Details The Study of the Early X-Ray Afterglows About Bright and Dark GRBs The Study of the Early X-Ray Afterglows About Bright and Dark GRBs

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007pnaoc...4..199l&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 4, No.

Astronomy and Astrophysics

Astronomy

X-Rays, Afterglow, Grb, Gamma-Ray Bursts

Scientific paper

A systematic study on the X-ray afterglows of the optically dark and bright gamma-ray bursts is presented. The results show that the distribution of the X-ray, the γ-ray of the dark GRBs and bright GRBs are similar, any observed differences should be caused by simply statistical fluctuation. These results indicated that the suppression of optical emission in the dark GRBs should result in the circumambiency, not in their central engine.

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