Pulses in gamma ray bursts

Details Pulses in gamma ray bursts Pulses in gamma ray bursts

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..366..187n&link_type=abstract

High velocity neutron stars and gamma-ray bursts. AIP Conference Proceedings, Volume 366, pp. 187-187 (1996).

Physics

Gamma-Ray Sources, Gamma-Ray Bursts, X-Ray

Scientific paper

If typical GRBs have X-ray counterparts similar to those detected by GINGA, then existing focussing X-ray telescopes will be able to detect GRBs three orders of magnitude fainter than the detection limit of BATSE. The EINSTEIN Observatory observed nearby galaxies for approximately 2 million seconds, during which time only one burstlike X-ray transient occurred. From this result we determine that GRBs cannot originate in a Galactic halo population with a limiting radius between 150 and 400 kpc. Inasmuch as halos with limiting radii outside of this range are excluded by BATSE isotropy measurements, our result indicates that all halo models are excluded.

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