High-velocity pulsars in the galactic halo

Details High-velocity pulsars in the galactic halo High-velocity pulsars in the galactic halo

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sci...257..937e&link_type=abstract

Science (ISSN 0036-8075), vol. 257, no. 5072, Aug. 14, 1992, p. 937-942. Research supported by USIBSF, DOE, and NSF.

Physics

49

Gamma Ray Bursts, Intergalactic Media, Interstellar Matter, Neutron Stars, Pulsars, White Dwarf Stars, Dark Matter, Galactic Halos, Massive Stars, Red Shift, Supernova Remnants

Scientific paper

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.

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