Ep-Eiso Correlation in a Multiple Subjet Model of Gamma-Ray Bursts

Details Ep-Eiso Correlation in a Multiple Subjet Model of Gamma-Ray Bursts Ep-Eiso Correlation in a Multiple Subjet Model of Gamma-Ray Bursts

2005-04-28

arxiv.org/abs/astro-ph/0504624v2

Astrophys.J.635:481,2005

Astronomy and Astrophysics

Astrophysics

9 pages, 7 figures; accepted for publication in ApJ

Scientific paper

10.1086/497388

We perform Monte Carlo simulations to study Ep-Eiso correlation in the context of a multiple subjet model (or inhomogeneous jet model) for gamma-ray bursts (GRBs), X-ray--rich GRBs (XRRs), and X-ray flashes (XRFs). For a single subjet, we find that Ep prop. Eiso^0.4 for large viewing angles. For the multiple subjet model in which all the subjets have the same intrinsic properties, off-axis events show Ep prop. Eiso^a with 0.4

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