activity
19992024
most citedModeling interaction of relativistic and nonrelativistic winds in binary system PSR 1259-63/SS2883. I.Hydrodynamical limit

144 citations · 945 across the 21 of their papers we have counts for

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8 papers · 1 filter

astro-ph2007★ 11 cited

Dissipationless Disk Accretion

Sergey V. Bogovalov, Stanislav R. Kelner

We consider disk accretion resulting purely from the loss of angular momentum due to the outflow of plasma from a magnetized disk. In this limiting case, the dissipation due to the…

astro-ph2007★ 144 cited

Modeling interaction of relativistic and nonrelativistic winds in binary system PSR 1259-63/SS2883. I.Hydrodynamical limit

S. V. Bogovalov, D. Khangulyan, A. V. Koldoba +2

In this paper, we present a detailed hydrodynamical study of the properties of the flow produced by the collision of a pulsar wind with the surrounding in a binary system. This wor…

astro-ph2006★ 126 cited

TeV lightcurve of PSR B1259-63/SS2883

Dmitry Khangulyan, Slavomir Hnatic, Felix Aharonian +1

The inverse Compton scattering of ultrarelativistic electrons accelerated at the pulsar wind termination shock is believed to be responsible for TeV gamma-ray signal recently repor…

astro-ph2002★ 80 cited

On the origin of the torus and jet-like structures in the centre of Crab Nebula

S. V. Bogovalov, D. V. Khangoulian

The formation of the toroidal and jet-like structures in the central part of the Crab Nebula is explained in the framework of Kennel & Coroniti theory. The only new element introdu…

astro-ph2002★ 47 cited

The Crab Nebula: interpretation of CHANDRA observations

S. V. Bogovalov, D. V. Khangoulyan

We interpret the observed X-ray morphology of the central part of the Crab Nebula (torus + jets) in terms of the standard theory by Kennel and Coroniti (1984). The only new element…

astro-ph2000★ 28 cited

Magnetocentrifugal acceleration of plasma in a nonaxisymmetric magnetosphere

S. V. Bogovalov

Violation of the axial synnetry of a magnetic field essentially modifies the physics of the plasma outflow in the magnetosphere of rotating objects. In comparison to the axisymmetr…