Ariel VI soft X-ray observations of Cygnus X-1

Details Ariel VI soft X-ray observations of Cygnus X-1 Ariel VI soft X-ray observations of Cygnus X-1

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...30..373b&link_type=abstract

(European Space Agency, ESLAB Symposium on X-ray Astronomy, 15th, Amsterdam, Netherlands, June 22-26, 1981.) Space Science Revie

Astronomy and Astrophysics

Astronomy

8

Ariel Satellites, Spaceborne Astronomy, Stellar Spectra, X Ray Astronomy, X Ray Sources, Cygnus Constellation, Energy Spectra, Radiant Flux Density, X Ray Stars

Scientific paper

Observations of Cygnus X-1 during the high-low transition of June-July 1980 reveal an intense flux between 0.5 and 1.5 keV. Although the intensity broadly follows the 1-12 keV flux through the transition, there is no evidence of variations in the shape of the energy spectrum. The implications of these results and derived limits on the minute-to-minute variability are discussed.

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