Astronomy and Astrophysics – Astrophysics
Scientific paper
1997-12-04
Astronomy and Astrophysics
Astrophysics
5 pages (aipproc LaTeX), 4 PostScript figures, to appear in Proceedings of the Fourth Compton Symposium, ed. C. D. Dermer, M.
Scientific paper
10.1063/1.53985
The hard X-ray emission from Cygnus X-1 has been monitored continually by BATSE since the launch of CGRO in April 1991. We present the hard X-ray intensity and spectral history of the source covering a period of more than five years. Power spectral analysis shows a significant peak at the binary orbital period. The 20-100 keV orbital light curve is roughly sinusoidal with a minimum near superior conjunction of the X-ray source and an rms modulation fraction of approximately 1.7%. No longer-term periodicities are evident in the power spectrum. We compare our results with other observations and discuss the implications for models of the source geometry.
Harmon Alan B.
McCollough Michael L.
Paciesas William
Robinson Craig Richard
Wilson Carol A.
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