Statistical study of high energy radiation from rotation-powered pulsars.

Details Statistical study of high energy radiation from rotation-powered pulsars. Statistical study of high energy radiation from rotation-powered pulsars.

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000sccha..43..171z&link_type=abstract

Science in China, Series A, Vol. 43, No. 2, p. 171 - 179

Other

Pulsars: Gamma Rays, Pulsars: X Rays

Scientific paper

Based on their self-consistent outer gap model for high energy emission from the rotation-powered pulsars, the authors study the statistical properties of X-ray and γ-ray emission from rotation-powered pulsars. Other statistical properties (e.g. diffuse γ-ray background and unidentified γ-ray point sources) related to γ-ray pulsars in our Galaxy and nearby galaxies are also considered.

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