The Early X-ray Afterglows of Optical Transient and Dark GRBs

Details The Early X-ray Afterglows of Optical Transient and Dark GRBs The Early X-ray Afterglows of Optical Transient and Dark GRBs

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..749l&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Physics

Scientific paper

We show that the distribution of the X-ray, the γ-ray and the fox of the dark GRBs and OT GRBs are similar; any observed differences should simply be due to statistical fluctuation. These results indicate that the suppression of optical emission in the dark GRBs should result from circumburst environment, not from their central engine.

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