4 citations · 5 across the 3 of their papers we have counts for
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On the contribution of the bow shock pulsar wind nebula PSR J0437-4715 to the observed fluxes of GeV-TeV positrons and antiprotons
A. E. Petrov, A. M. Bykov
The orbital observatories PAMELA and AMS-02 have detected a significant excess in the cosmic ray (CR) positron flux at energies above several tens of GeV. The measured values excee…
How many VHE gamma-ray binaries with young pulsars can be observed?
A. M. Bykov, A. G. Kuranov, A. E. Petrov +1
A population of Galactic gamma-ray binaries is currently emerging due to ever increasing sensitivity of gamma-ray observatories. The detection of very high energy (VHE) photons wit…
Relativistic astrospheres of gamma-ray binaries: modeling of non-thermal processes
A. M. Bykov, A. E. Petrov, K. P. Levenfish
A long standing problem in high energy astrophysics is the nature of galactic accelerators of particles with energies above PeV. Such objects are sources of galactic cosmic rays an…
PeV proton acceleration in Gamma-ray Binaries
A. M. Bykov, A. E. Petrov, G. A. Ponomaryov +2
Current generation of ground based gamma-ray telescopes observed dozens of sources of photons above 100 TeV. Supernova remnants, pulsar wind nebulae, young stellar clusters and sup…