Disk plus halo models of gamma-ray burst sources

Details Disk plus halo models of gamma-ray burst sources Disk plus halo models of gamma-ray burst sources

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...410l..23s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 410, no. 1, p. L23-L26.

Astronomy and Astrophysics

Astrophysics

45

Astronomical Models, Galactic Halos, Gamma Ray Bursts, Cyclotron Radiation, Dark Matter, Luminosity, Neutron Stars

Scientific paper

The present consideration of Gaussian halo, exponential halo, and standard 'dark matter' halo forms for the distribution of Galactic halo sources indicates that about 70 percent of the gamma-ray bursts observed by the BATSE program can come from local Galactic disk neutron stars, with the rest lying in an extended Galactic halo. Two specific disk-halo combinations are considered as examples which use an exponential disk; in the first case, this is combined with a Gaussian halo, and in the second, with a dark matter halo.

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