Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-12-02
Astronomy and Astrophysics
Astrophysics
22 pages, including 6 figures; uses epsf.sty, rotate.sty; now accepted for publication in ApJ; significant modifications of te
Scientific paper
We use a new method of analysis to determine parameters of cosmological gamma-ray bursts (GRBs), assuming that their distribution follows the star-formation history of the universe. Spectral evolution is calculated from an external shock model for fireball/blast wave evolution, and used to evaluate the measured peak flux, duration, and $\nu F_\nu$ peak photon energy for a GRB source occuring at a given redshift and with given values of total energy, baryon-loading and environmental parameters. We then fit model distributions of GRB sources to the observed peak flux, duration and $\nu F_\nu$ peak photon energy distributions. We find that the observed width of the $E_p$ and duration distributions can not be explained by cosmological redshift and time dilation effects. Rather, broad distributions of total blastwave energies and bulk Lorentz factors are necessary to explain the observed distributions simultaneously within the framework of our unifying GRB model. We discuss implications for source parameter distributions and determine a range of burst parameters consistent with the data.
Boettcher Markus
Dermer Carles D.
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