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Gamma-ray bursts from high velocity neutron stars
Authors:Tomasz Bulik  Donald Q Lamb
Institution:(1) Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, 60637 Chicago, IL, USA
Abstract:We investigate the viability of the Galactic corona model of gamma-ray bursts by calculating the spatial distribution of neutron stars born with high velocities in the Galactic disk, and comparing the resulting brightness and angular distribution with the BATSE data. We find that the Galactic corona model can reproduce the BATSE peak flux and angular distribution data for neutron star kick velocities gap 800 km s–1, source turn-on ages gap 10 Myrs, and sampling depths 100 kpc lapd maxlap 400 kpc.
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