High-Velocity Pulsars in the Galactic Halo
David Eichler 1 and
Joseph Silk 2
1 Department of Physics, Ben Gurion University, Beer Sheva, Israel
2 Departments of Astronomy and Physics and Center for Particle Astrophysics, University of California, Berkeley, CA 94720
It is proposed that high-velocity pulsars are produced in extended galactic halos, and possibly in extragalactic space, from primordial (population III) stars. Such a population of neutron stars could provide an explanation for the gamma-ray bursters and would then accommodate the possibility that most bursters are not in the visible parts of galaxies.
Submitted on February 12, 1992
Accepted on June 23, 1992