336 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Max Planck Institute for Nuclear PhysicsDE30 papers
- Max Planck SocietyDE20 papers
- Russian Academy of SciencesRU8 papers
- Institute for Nuclear ResearchRU6 papers
- Siberian Branch of the Russian Academy of SciencesRU3 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TorinoIT2 papers
- Kavli Institute for the Physics and Mathematics of the UniverseJP2 papers
- Lomonosov Moscow State UniversityRU2 papers
- National Institute for AstrophysicsIT2 papers
- New York UniversityUS2 papers
- North Carolina State UniversityUS2 papers
- Norwegian University of Science and TechnologyNO2 papers
8 papers · 1 filter
Nonthermal and thermal emission from the supernova remnant RX J1713.7-3946
E. G. Berezhko, H. J. Voelk
A nonlinear kinetic theory of cosmic ray (CR) acceleration in supernova remnants (SNRs) is employed to investigate the properties of SNR RX J1713.7-3946. Observations of the non-th…
Constraints on the flux of primary cosmic-ray photons at energies E > 10^18 eV from Yakutsk muon data
A. V. Glushkov, I. T. Makarov, M. I. Pravdin +4
Comparing the signals measured by the surface and underground scintillator detectors of the Yakutsk Extensive Air Shower Array, we place upper limits on the integral flux and the f…
Theory of cosmic ray and gamma-ray production in the supernova remnant RX J0852.0-4622
E. G. Berezhko, G. Pühlhofer, H. J. Völk
Aims. The properties of the Galactic supernova remnant (SNR) RX J0852.0-4622 are theoretically analysed. Methods. An explicitly time-dependent, nonlinear kinetic model of cosmic ra…
Cosmic ray acceleration parameters from multi-wavelength observations. The case of SN 1006
E. G. Berezhko, L. T. Ksenofontov, H. J. Voelk
The properties of the Galactic supernova remnant SN 1006 are theoretically reanalysed. Nonlinear kinetic theory is used to determine the acceleration efficiency of cosmic rays (CRs…
Composition of cosmic rays accelerated in active galactic nuclei
E. G. Berezhko
The composition of the overall spectrum of cosmic rays (CRs) is studied under the assumption that ultra high energy CRs above the energy 10^{17} eV are produced at the shock create…
Exploring arrival directions of UHECRs with the Yakutsk array
A. A. Ivanov
The data on arrival directions of ultra-high energy cosmic rays (UHECRs) detected with the Yakutsk array are analyzed. The work is induced by the recent claim of the Pierre Auger c…
Galactic origin of ultrahigh energy cosmic rays
A. A. Mikhailov
The arrival directions of ultrahigh energy extensive air showers (EAS) by Yakutsk, AGASA, P. Auger array data are analyzed. For the first time, the maps of equal exposition of cele…
Measuring extensive air showers with Cherenkov light detectors of the Yakutsk array: The energy spectrum of cosmic rays
A. A. Ivanov, S. P. Knurenko, I. Ye. Sleptsov
The energy spectrum of cosmic rays in the range 10^15 eV to 6*10^19 eV has been studied using the air Cherenkov light detectors of the Yakutsk array. The total flux of photons prod…