COS-B X-ray observations of Cygnus X-3

Details COS-B X-ray observations of Cygnus X-3 COS-B X-ray observations of Cygnus X-3

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....62..275b&link_type=abstract

Astronomy and Astrophysics, vol. 62, no. 1-2, Jan. 1978, p. 275, 276. Research supported by the Comitato Regionale Siciliano pe

Astronomy and Astrophysics

Astronomy

7

Cos-B Satellite, Spaceborne Astronomy, X Ray Sources, Gamma Ray Astronomy, Light Curve, Modulation, Radiant Flux Density, Variable Stars

Scientific paper

The ESA COS-B satellite has observed the Cygnus region in the energy
range (2-12 keV), between 1975 November 28.42 and December 24.26. The
Cygnus X-3 4.8 h modulation is detected. The source was in a low state
with a positive evidence for an increase in flux during the month of
observation.

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