The intrinsic gamma ray burst luminosity function from observational data analysis

Details The intrinsic gamma ray burst luminosity function from observational data analysis The intrinsic gamma ray burst luminosity function from observational data analysis

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115..426b&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 426-428 (1984).

Physics

5

X-Ray Sources, X-Ray Bursts

Scientific paper

The spatial distribution of the gamma ray bursts, selected according to their spectral hardness, appear spherical with divergence from an isotropic behavior depending on the spectral parameter KT. This can be explained by an intrinsic luminosity function and a disk or halo galactic distribution. If we assume a galactic disk distribution we derive an average peak burst luminosity of 1039 erg/sec.

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