Pulsars and the Distribution of Celestial Gamma Rays

Details Pulsars and the Distribution of Celestial Gamma Rays Pulsars and the Distribution of Celestial Gamma Rays

Aug 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970phrvl..25..603p&link_type=abstract

Physical Review Letters, vol. 25, Issue 9, pp. 603-605

Physics

20

Scientific paper

The flux of celestial gamma rays from discrete sources (for example, pulsars) is calculated, showing that these sources emit fluxes of several 10-6 quanta/cm2 sec over regions of several tens of degrees (among them Vela X). Hence they should be observable. The calculations show further that the high gamma-ray flux values of OSO-III follow from the expected correlation of cosmic-ray sources with regions of large hydrogen density.

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