X-ray observations of the variability of Cygnus X-1 in the high state

Details X-ray observations of the variability of Cygnus X-1 in the high state X-ray observations of the variability of Cygnus X-1 in the high state

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....62..265m&link_type=abstract

Astronomy and Astrophysics, vol. 62, no. 1-2, Jan. 1978, p. 265, 266. Research supported by the Comitato Regionale Siciliano per

Astronomy and Astrophysics

Astronomy

Cos-B Satellite, Light Curve, Spaceborne Astronomy, Variable Stars, X Ray Sources, Ariel Satellites, Satellite-Borne Instruments

Scientific paper

The ESA COS-B satellite has observed the Cygnus region in the energy range 2-12 keV, between November 28 and December 24, 1975. The Cygnus X-1 X-ray light curve for this period, during which the source appears to be in the high state, is reported; a search for a possible attenuation of the X-ray emission at the superior conjunction brings to the conclusion that the evidence for the existence of such a feature is dubious.

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