Two Classes of Gamma-Ray Bursts
Astrophysics
2007-05-23 v1
Abstract
Data from the 3B Catalogue suggest that short and long GRB are the results of different classes of events, rather than different parameter values within a single class: Short bursts have harder spectra in the BATSE bands, but chiefly long bursts are detected at photon energies over 1 MeV, implying that their hard photons are radiated by a process not found in short bursts. The values of \langle V/V_{max} \rangle for short and long bursts differ by 4.3 \sigma, implying different spatial distributions. Only the soft gamma-ray radiation mechanisms are the same in both classes.
Keywords
Cite
@article{arxiv.astro-ph/9512074,
title = {Two Classes of Gamma-Ray Bursts},
author = {J. I. Katz and L. M. Canel},
journal= {arXiv preprint arXiv:astro-ph/9512074},
year = {2007}
}
Comments
6pp, tex, no figures