Second variation of Cygnus X-1 in hard X-rays

Details Second variation of Cygnus X-1 in hard X-rays Second variation of Cygnus X-1 in hard X-rays

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cosp.meet.....n&link_type=abstract

COSPAR, Plenary Meeting, 21st, Innsbruck, Austria, May 29-June 10, 1978, Paper. 14 p.

Physics

Variable Stars, X Ray Sources, Balloon-Borne Instruments, Fourier Transformation, Time Series Analysis

Scientific paper

The Fourier analysis method is applied to hard X-ray data obtained from Cyg X-1 with balloon-borne detectors. Power spectrum densities are determined for the OFF and ON states, and it is found that the power spectrum density exhibits a significant (99.7%) peak at about 0.052 Hz for the ON state but not for the OFF state. The results suggest that 24% of the hard X-ray intensity of Cyg X-1 is variable with a period of 19.2 sec.

Affiliated with

Also associated with

No associations

Rating

Second variation of Cygnus X-1 in hard X-rays does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Second variation of Cygnus X-1 in hard X-rays, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Second variation of Cygnus X-1 in hard X-rays will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1296248