z-logo
open-access-imgOpen Access
Spectra of Unsteady Wind Models of Gamma-Ray Bursts
Author(s) -
H. Papathanassiou,
P. Mészáros
Publication year - 1996
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310343
Subject(s) - physics , particle acceleration , spectral line , gamma ray burst , radiation , range (aeronautics) , event (particle physics) , photon , astrophysics , computational physics , acceleration , wavelength , nuclear physics , optics , astronomy , classical mechanics , materials science , composite material
We calculate the spectra expected from unsteady relativistic wind models ofgamma-ray bursts, suitable for events of arbitrary duration. The spectralenergy distribution of the burst is calculated over photon energies spanningfrom eV to TeV, for a range of event durations and variability timescales. Therelative strength of the emission at different wavelengths can provide valuableinformation on the particle acceleration, radiation mechanisms and the possibletypes of models.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom