32 citations · 56 across the 6 of their papers we have counts for
6 papers
Shells and bubbles around compact clusters of massive stars: 3D MHD simulations
D. V. Badmaev, A. M. Bykov, M. E. Kalyashova
We present the results of three-dimensional magnetohydrodynamic (3D MHD) simulations of the plasma flow structure in the vicinity of a compact cluster of young massive stars. The c…
An Approach to Gamma-Hadron Separation via Measurements of the Middle-UV Fraction of EAS emission by an Imaging Atmospheric Cherenkov Telescope with UV-Sensitive SiPM detectors
E. E. Kholupenko, D. V. Badmaev, N. M. Budnev +7
The operation of a small-size Cherenkov gamma-ray telescope TAIGA-IACT with camera on SiPMs OnSemi MicroFJ-60035 has been modelled by multiparticle Monte Carlo (MC) methods. The mo…
Core-collapse supernova inside the core of a young massive star cluster: 3D MHD simulations
D. V. Badmaev, A. M. Bykov, M. E. Kalyashova
Young massive stars in compact stellar clusters could end their evolution as core-collapse supernovae a few million years after the cluster was built. The blast wave of a supernova…
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…
Inside the core of a young massive star cluster: 3D MHD simulations
D. V. Badmaev, A. M. Bykov, M. E. Kalyashova
Young massive star clusters inhabit regions of star formation and play an essential role in the galactic evolution. They are sources of both thermal and non-thermal radiation, and…
Wolf-Rayet stars in young massive star clusters as potential sources of Galactic cosmic rays
Maria E Kalyashova, Andrei M Bykov, Sergei M Osipov +2
For most elements, the isotopic ratios seen in cosmic rays (CRs) are similar to those in the solar wind. The most important exception to this is Ne/Ne where the CR va…