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Production of neutrons, neutrinos and gamma-rays by a very fast pulsar in the Galactic Center region
W. Bednarek
We consider the possibility that the excess of cosmic rays near eV, reported by the AGASA and SUGAR groups from the direction of the Galactic Center, is caused by a…
Extragalactic neutrino background from very young pulsars surrounded by supernova envelopes
W. Bednarek
We estimate the extragalactic muon neutrino background which is produced by hadrons injected by very young pulsars at an early phase after supernova explosion. It is assumed that h…
Neutrinos from Early-Phase, Pulsar-Driven Supernovae
J. H. Beall, W. Bednarek
Neutron stars, just after their formation, are surrounded by expanding, dense, and very hot envelopes which radiate thermal photons. Iron nuclei can be accelerated in the wind zone…
Contribution of nuclei accelerated by gamma-ray pulsars to cosmic rays in the Galaxy
W. Bednarek, R. J. Protheroe
We consider the galactic population of gamma-ray pulsars as possible sources of cosmic rays at and just above the ``knee'' in the observed cosmic ray spectrum at --$10^{16…
Propagation of gamma-rays in massive binary Cen X-3: Interaction of cascade gamma-rays with the massive star
W. Bednarek
We consider the propagation of very high energy (VHE) gamma-rays in the radiation field of the massive star of binary system Cen X-3. VHE gamma-rays or electrons, injected by the c…