activity
20042024
most citedDots, clumps and filaments: the intermittent images of synchrotron emission in random magnetic fields of young supernova remnants

81 citations · 283 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2024★ 9 cited

X-ray polarization: A view deep inside cosmic ray driven turbulence and particle acceleration in supernova remnants

Andrei. M. Bykov, Sergei. M. Osipov, Yury. A. Uvarov +2

We show here that highly polarized X-ray synchrotron radiation from young supernova remnants (SNRs) can be modeled within the framework of diffusive shock acceleration (DSA) and no…

astro-ph.HE2023★ 9 cited

X-ray emission from Westerlund 2 detected by SRG/ART-XC and Chandra: search for radiation of TeV leptons

A. M. Bykov, Yu. A. Uvarov, M. E. Kalyashova +5

We present the results of current observations of the young compact cluster of massive stars Westerlund 2 with the Mikhail Pavlinsky ART-XC telescope aboard the Spectrum-Roentgen-G…

astro-ph.GA2021★ 3 cited

Spatially resolved X-ray spectra of the Galactic SNR G18.95-1.1: SRG/eROSITA view

A. M. Bykov, Y. A. Uvarov, E. M. Churazov +2

Aims. We study the X-ray emission of the galactic supernova remnant (SNR) G18.95-1.1 with the eROSITA telescope on board the Spectrum Rentgen Gamma (SRG) orbital observatory. In ad…

astro-ph.HE2020★ 18 cited

Uncovering magnetic turbulence in young supernova remnants with polarized X-ray imaging

Andrei M. Bykov, Yury A. Uvarov, Patrick Slane +1

Observations of young supernova remnants (SNRs) in X-rays and gamma-rays have provided conclusive evidence for particle acceleration to at least TeV energies. Analysis of high spat…

astro-ph.HE2020★ 11 cited

Gamma-ray flux depressions of the Crab nebula in the high-energy range

M. S. Pshirkov, B. A. Nizamov, A. M. Bykov +1

The giant gamma-ray flares of the Crab nebula discovered by AGILE and Fermi observatories came as a surprise and have challenged the existing models of pulsar wind nebulae. We have…

astro-ph.HE2016★ 1 cited

Unveiling the Magnetic Structure of VHE SNRs/PWNe with XIPE, the X-ray Imaging-Polarimetry Satellite

E. de Ona Wilhelmi, J. Vink, A. Bykov +6

The dynamics, energetics and evolution of pulsar wind nebulae (PWNe) and supernova remnants (SNRs), are strongly affected by their magnetic field strength and distribution. They ar…