High energy gamma-rays from Cygnus X-3

Details High energy gamma-rays from Cygnus X-3 High energy gamma-rays from Cygnus X-3

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989acaps...9..286l&link_type=abstract

(Acta Astrophysica Sinica, vol. 9, no. 3, 1989, p. 286-288) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, Dec. 1

Astronomy and Astrophysics

Astronomy

Gamma Ray Astronomy, Radiant Flux Density, X Ray Binaries, Esa Satellites, Maximum Entropy Method, X Ray Astronomy

Scientific paper

The maximum entropy method of image analysis has been improved and applied to high-energy gamma-rays from Cygnus X-3 during three periods when the X-ray emission was high. The results show that the 2-12 keV X-rays and 150-5000 MeV gamma rays from Cyg X-3 are negatively correlated. A clear gamma-ray image of Cyg-X-3 can be obtained between June 1977 and June 1980, when the X-ray emission was low. A flux of about 10 to the - 6th/sq cm/s was obtained.

Affiliated with

Also associated with

No associations

Rating

High energy gamma-rays from 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 High energy gamma-rays from Cygnus X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High energy gamma-rays from Cygnus X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1565293