Hard X-ray fluxes in the energy range from 40 to 290 keV

Details Hard X-ray fluxes in the energy range from 40 to 290 keV Hard X-ray fluxes in the energy range from 40 to 290 keV

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pazh....1....6b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 1, June 1975, p. 6-11. In Russian.

Astronomy and Astrophysics

Astronomy

3

Astronomical Spectroscopy, Cosmos Satellites, Galactic Structure, X Ray Astronomy, Radiant Flux Density, Scintillation Counters, Spaceborne Astronomy

Scientific paper

Preliminary results are reported for analysis of hard X-ray flares detected by a scintillation spectrometer on board Cosmos 428. It is shown that the number of flares with shorter duration was greater than that with longer duration and that the shorter flares had correspondingly lesser energy fluxes. The integral distribution of the number of flares is plotted as a function of energy flux and galactic latitude. It is found that the results do not contradict the law of homogeneous source-density distribution in space, but that a distribution along the galactic disk cannot be excluded at this time.

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