Bykov Andrey M.
  • Affiliation
    Ioffe Institute
  • St. Petersburg, Russian Federation

A new class of galactic X-ray sources resulting from interaction of stellar wind with a supernova remnant

Astrophysics
  • Year: 2011
  • Issue: 1
  • 0
  • 5405
  • Pages: 106-110

Spectral diagnostics of the interstellar radiative shocks

Astrophysics
  • Year: 2011
  • Issue: 2
  • 0
  • 5508
  • Pages: 150-157

A search for radio nebulae around pulsars PSR J0358+5413, PSR J1809-1917 and PSR В1800-21

Astrophysics
  • Year: 2011
  • Issue: 3
  • 0
  • 5530
  • Pages: 176-182

The influence of the night-sky background on ground-based observations of gamma-ray bursts in the range between 1 and 10 GeV

Astrophysics
  • Year: 2012
  • Issue: 3
  • 0
  • 5535
  • Pages: 191-195

Vela pulsar wind nebula: determination of the anisotropy of accelerated particle distribution function

Astrophysics
  • Year: 2012
  • Issue: 3
  • 0
  • 5299
  • Pages: 201-210

Role of firehose instability in diffusive shock acceleration

Astrophysics
  • Year: 2012
  • Issue: 3
  • 0
  • 5516
  • Pages: 195-201

The spatial distribution features of Сherenkov photon flux in the core of an electron-photon extensive atmospheric shower induced by a 5 GeV primary gamma-quantum

Simulation of physical processes
  • Year: 2011
  • Issue: 4
  • 1
  • 5581
  • Pages: 79-86

Asymmetry study of the mixed-morphology supernova remnant G 18.95-1.1

Astrophysics
  • Year: 2023
  • Volume: 16
  • Issue: 1.2
  • 0
  • 943
  • Pages: 362-369

Kinetic modeling of MHD parameters of mildly-relativistic shocks

Astrophysics
  • Year: 2023
  • Volume: 16
  • Issue: 1.2
  • 7
  • 887
  • Pages: 461-466