Long-period gamma-ray variability of Cygnus X-3

Details Long-period gamma-ray variability of Cygnus X-3 Long-period gamma-ray variability of Cygnus X-3

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..452n&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, June 1986, p. 452-457) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, May-June

Astronomy and Astrophysics

Astronomy

2

Cygnus Constellation, Gamma Rays, Periodic Variations, Variable Stars, X Ray Stars, Cerenkov Radiation, Histograms, Statistical Analysis, Time Dependence

Scientific paper

Data from the Crimean Astrophysical Observatory (CAO) and other facilities on the ultrahigh-energy (E greater than or equal to 2 x 10 to the 12th eV) gamma rays coming from the direction of the Cyg X-3 source are analyzed. Histograms are presented for the gamma-ray signal/noise ratio as a function of phase of candidate 328- and 19.58-day variability periods. Good agreement between CAO and T'ien Shan station data confirms the presence of a cycle in the ultrahigh-energy gamma-ray flux with a period of 19.58 + or - 0.02 days.

Affiliated with

Also associated with

No associations

Rating

Long-period gamma-ray variability of Cygnus X-3 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 Long-period gamma-ray variability of Cygnus X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Long-period gamma-ray variability of Cygnus X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1834004