X-ray source counts at high galactic latitude

Details X-ray source counts at high galactic latitude X-ray source counts at high galactic latitude

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183..169w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, Apr. 1978, p. 169-175.

Astronomy and Astrophysics

Astronomy

21

Luminous Intensity, Satellite Observation, Spatial Distribution, X Ray Sources, Ariel 5 Satellite, Computerized Simulation, Euclidean Geometry, Galactic Radiation, Monte Carlo Method, Spaceborne Astronomy

Scientific paper

The Ariel V Catalogue is used to investigate the number-intensity
distribution of X-ray sources at high galactic latitude. The results are
consistent with a uniform distribution of sources in Euclidean space.

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