activity
20052024
most citedMonotonic and cyclic components of radio pulsars spin-down

33 citations · 226 across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.HE2024★ 3 cited

Evidence for the spin-kick alignment of pulsars from the statistics of their magnetic inclinations

Anton Biryukov, Gregory Beskin

It is thought that isolated neutron stars receive a natal kick velocity at birth nearly aligned with their spin axis. Direct observational confirmation of this alignment is current…

astro-ph.IM2023

SAINT (Small Aperture Imaging Network Telescope) -- a wide-field telescope complex for detecting and studying optical transients at times from milliseconds to years

Grigory Beskin, Anton Biryukov, Alexey Gutaev +7

(Abridged) In this paper, we present a project of multi-channel wide-field optical sky monitoring system with high temporal resolution -- Small Aperture Imaging Network Telescope (…

astro-ph.HE2023★ 3 cited

Imprint of magnetic obliquity in apparent spin-down of radio pulsars

Anton Biryukov, Gregory Beskin

Numerical simulations predict that the spin-down rate of a single rotation-powered neutron star depends on the angle between its spin and magnetic axes as $P\dot P \propto μ^2…

astro-ph.HE2022★ 2 cited

Observability of isolated neutron stars at SRG/eROSITA

A. D. Khokhriakova, A. V. Biryukov, S. B. Popov

A four-year sky survey with the use of the eROSITA telescope on board the Spektr-RG observatory will provide the best coverage in the soft (0.5-2 keV) and standard (2-10 keV) X-ray…

astro-ph.HE2021★ 16 cited

Exceptionally bright optical emission from a rare and distant ray burst

Gor Oganesyan, Sergey Karpov, Martin Jelínek +19

Long -ray bursts (GRBs) are produced by the dissipation of ultra-relativistic jets launched by newly-born black holes after the collapse of massive stars. Right after the lu…

astro-ph.HE2021★ 25 cited

Magnetic angle evolution in accreting neutron stars

Anton Biryukov, Pavel Abolmasov

The rotation of a magnetised accreting neutron star (NS) in a binary system is described by its spin period and two angles: spin inclination with respect to the orbital momentu…