The cycle-to-cycle variability of Cygnus X-3

Details The cycle-to-cycle variability of Cygnus X-3 The cycle-to-cycle variability of Cygnus X-3

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...50..129v&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 50, Oct. 1982, p. 129-140. Research supported by the Nederlandse Organisatie

Astronomy and Astrophysics

Astrophysics

12

Binary Stars, Light Curve, Statistical Analysis, Variable Stars, X Ray Sources, Orbits, Signal To Noise Ratios, Stellar Structure

Scientific paper

Results are reported of a study of the variability of the shape of the light curve of Cyg X-3 from one cycle to the next on time scales down to about 200 s. Variations occur mainly around the maximum of the light curve, on a time scale of about half an hour or less, and give rise to a dispersion of the individual light curves around the mean which is a considerable fraction of the amplitude of the modulation.

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