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20172026
most citedShocks and non-thermal particles in clusters of galaxies

50 citations · 61 across the 4 of their papers we have counts for

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5 papers · 1 filter

astro-ph.HE20264 cited

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…

astro-ph.HE20245 cited

Cosmic ray acceleration and non-thermal emission from fast luminous optical transient sources

V. I. Romansky, A. M. Bykov, S. M. Osipov

Fast blue optical transients (FBOTs) represent a new class of highly energetic sources observed from radio to X-rays. High luminosity, light curves and spectra of the sources can b…

astro-ph.HE2024

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…

astro-ph.HE201950 cited

Shocks and non-thermal particles in clusters of galaxies

A. M. Bykov, F. Vazza, J. A. Kropotina +2

Galaxy clusters grow by gas accretion, mostly from mergers of substructures, which release powerful shock waves into cosmic plasmas and convert a fraction of kinetic energy into th…

astro-ph.HE2017

Pulsar wind nebulae with bow shocks: non-thermal radiation and cosmic ray leptons

A. M. Bykov, E. Amato, A. E. Petrov +2

Pulsars with high spin-down power produce relativistic winds radiating a fraction of the power in the range from radio to gamma-rays in the pulsar wind nebulae (PWNe). The rest of…