120 citations · 616 across the 30 of their papers we have counts for
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Secondary cosmic-ray nuclei in the Galactic halo model with nonlinear Landau damping
D. O. Chernyshov, A. V. Ivlev, V. A. Dogiel
We employed our recent model of the cosmic-ray (CR) halo to compute the Galactic spectra of stable and unstable secondary nuclei. In this model, confinement of the Galactic CRs is…
Formation of the cosmic-ray halo: The role of nonlinear Landau damping
D. O. Chernyshov, V. A. Dogiel, A. V. Ivlev +2
We present a nonlinear model of self-consistent Galactic halo, where the processes of cosmic ray (CR) propagation and excitation/damping of MHD waves are included. The MHD-turbulen…
Self-modulation of cosmic rays in molecular clouds: Imprints in the radio observations
V. A. Dogiel, D. O. Chernyshov, A. V. Ivlev +2
We analyze properties of non-thermal radio emission from the Central Molecular Zone (CMZ) and individual molecular clouds, and argue that the observed features can be interpreted i…
Fermi bubbles as a source of cosmic rays above 10^{15} eV
D. O. Chernyshov, K. S. Cheng, V. A. Dogiel +1
Fermi bubbles are giant gamma-ray structures extended north and south of the Galactic center with characteristic sizes of order of 10 kpc recently discovered by Fermi Large Area Te…
Multi-wavelength Emission from the Fermi Bubble II. Secondary Electrons and the Hadronic Model of the Bubble
K. -S. Cheng, D. O. Chernyshov, V. A. Dogiel +1
We analyse the origin of the gamma-ray flux from the Fermi Bubbles (FBs) in the framework of the hadronic model in which gamma-rays are produced by collisions of relativistic proto…
Multi-wavelength Emission from the Fermi Bubble I. Stochastic acceleration from Background Plasma
K. S. Cheng, D. O. Chernyshov, V. A. Dogiel +1
We analyse processes of electron acceleration in the Fermi Bubbles in order to define parameters and restrictions of the models, which are suggested for the origin of these giant r…