Hard X-ray observations near Ariel 1118-61

Details Hard X-ray observations near Ariel 1118-61 Hard X-ray observations near Ariel 1118-61

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.256..292c&link_type=abstract

Nature, vol. 256, July 24, 1975, p. 292, 293.

Other

3

Black Body Radiation, Variable Stars, X Ray Sources, Ariel Satellites, Energy Spectra, Photons

Scientific paper

Observations made by Ariel V in the region of Cen X-3 have revealed a new transient X-ray source with a periodicity of 6.75 min. In addition to proportional counter observations during the period December 17, 1974 to January 31, 1975, the Imperial College crystal scintillator, sensitive to the photon energy range 26 keV to 1.2 MeV, viewed the same region of the sky. A source a few degrees from the direction of the spin axis can be detected by determining the modulation in the counting rate seen in four equal angle spin sectors with a time resolution of 512 s. The satellite observations are compared with results reported by other workers and it is concluded that a black body radiation from a low skin depth gas is the most likely single source mechanism.

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