Gamma-Rays from the Close Massive Binary Cyg X-3

Details Gamma-Rays from the Close Massive Binary Cyg X-3 Gamma-Rays from the Close Massive Binary Cyg X-3

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2477s&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Some observations indicate the existence of an energetic pulsar in the massive binary Cyg X-3. We assume that such a pulsar injects relativistic e± pairs which propagate radially in the pulsar wind zone. These e± pairs initiate inverse Compton e± pair cascade in a very strong anisotropic radiation field of the Wolf-Rayet star. We calculate the expected phase dependent gamma-ray spectra produced in such a cascade.

Affiliated with

Also associated with

No associations

Rating

Gamma-Rays from the Close Massive Binary Cyg 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 Gamma-Rays from the Close Massive Binary Cyg X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-Rays from the Close Massive Binary Cyg X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1141633