144 citations · 945 across the 21 of their papers we have counts for
21 papers
Waves in strong centrifugal filed: dissipative gas
S. V. Bogovalov, V. A. Kislov, I. V. Tronin
In the fast rotating gas (with the velocity typical for Iguassu gas centrifuge) three families of linear waves exist with different polarizations and law of dispersion. The energy…
Modelling the interaction between relativistic and non-relativistic winds in binary pulsar systems: strong magnetization of the pulsar wind
Sergey V. Bogovalov, Dmitry Khangulyan, Alexander V. Koldoba +2
We present a numerical study of the properties of the flow produced by the collision of a magnetized anisotropic pulsar wind with the circumbinary environment. We focus on studying…
Magnetic absorption of VHE photons in the magnetosphere of the Crab pulsar
S. V. Bogovalov, I. Contopoulos, A. Prosekin +2
The detection of the pulsed ~TeV gamma-ray emission from the Crab pulsar reported by MAGIC and VERITAS collaborations demands a substantial revision of existing models of…
Ratio of kinetic luminosity of the jet to bolometric luminosity of the disk at the "cold" accretion onto a supermassive black hole
S. V. Bogovalov
Disk accretion onto black holes is accompanied by collimated outflows (jets). In active galactic nuclei (AGN), the kinetic energy flux of the jet may exceed the bolometric luminosi…
Dependence of the separative power of an optimised Iguassu gas centrifuge on the velocity of rotor
S. V. Bogovalov, V. D. Borman, V. D. Borisevich +2
Purpose - The purpose of this work is to determine dependence of the separative power of the Iguassu gas centrifuge (GC) on the velocity of the rotor. Design/methodology/approach -…
On the anomalously large extension of the Pulsar Wind Nebula HESS J1825-137
Dmitry Khangulyan, Alexander V. Koldoba, Galina V. Ustyugova +2
The very high energy (VHE) gamma-ray emission reported from a number of pulsar wind nebulae (PWNe) is naturally explained by the inverse Compton scattering of multi-TeV electrons.…