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An Interpretation of the hνpeak - Eiso Correlation for GRB

David Eichler, Amir Levinson

astro-pharXiv:astro-ph/0405014

Abstract

The hνpeak/100 KeV [Eiso/1052 erg]1/2 correlation reported recently by Amati et al. (2002) and Lamb et al. (2003) for long GRB's can be interpreted as a viewing angle effect if the emitting region of the fireball is ring-shaped.

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