Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2485b&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
1
Scientific paper
We consider propagation of relativistic heavy nuclei injected by a young pulsar into the radiation field of a massive companion. If the binary system is close enough, then the nuclei suffer multiple photo desintegrations in collisions with thermal photons coming from the massive star. Some neutrons and charged particles, which are dissolved from the nuclei, can collide with the massive star producing neutrinos. We calculate neutrino fluxes for different impact parameters of particles onto the massive star applying as an example the parameters of the Cyg X-3 system.
Bartosik Marek
Bednarek Wlodek
Sierpowska Agnieszka
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