An Interpretation of the hν_(peak) - E_(iso) Correlation for GRB
classification
🌌 astro-ph
keywords
correlationpeakamatiangleeffectemittingfireballinterpretation
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The $h\nu_{peak}/100 KeV \sim [E_{iso}/10^{52} \rm{erg}]^{1/2}$ 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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