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pro vyhledávání: '"Kuzyo, T"'
The three-dimensional velocity structure of the shock-heated Si-reach and S-reach ejecta were reconstructed in Tycho supernova remnant from Doppler-shifted lines. The vector components along the line of sight were restored from the spatially resolved
Externí odkaz:
http://arxiv.org/abs/2412.04096
Autor:
Petruk, O., Kuzyo, T.
Publikováno v:
A&A 688, A108 (2024)
The momentum distribution of particles accelerated at strong non-relativistic shocks may be influenced by the spatial distribution of the flow speed around the shock. This phenomenon becomes evident in the cosmic-ray modified shock, where the particl
Externí odkaz:
http://arxiv.org/abs/2404.17397
Supernova remnants (SNRs) can be rich sources of information on the parent SN explosion. Thus investigating the transition from the phase of SN to that of SNR can be crucial to link these two phases of evolution. Here we aim to study the early develo
Externí odkaz:
http://arxiv.org/abs/2105.02938
Autor:
Petruk, O., Kuzyo, T., Orlando, S., Pohl, M., Miceli, M., Bocchino, F., Beshley, V., Brose, R.
We present very-high-resolution 1D MHD simulations of the late-stage supernova remnants (SNR). In the post-adiabatic stage the magnetic field has an important and significant dynamical effect on the shock dynamics, the flow structure, and hence the a
Externí odkaz:
http://arxiv.org/abs/1806.11396
Gamma-rays from hadronic collisions are expected from supernova remnants (SNRs) located near molecular clouds. The temperature on the shock interacting with the dense environment quickly reaches $10^5$ K. The radiative losses of plasma become essenti
Externí odkaz:
http://arxiv.org/abs/1511.06156
Images of SN1006 have a number of important properties. For instance, the bright limbs coincide spatially in various bands, they have different brightness, and the contrast of brightness varies from radio to gamma-rays. The reasons of such properties
Externí odkaz:
http://arxiv.org/abs/1109.0831
Akademický článek
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Astronomy and astrophysics 634, A59 - (2020). doi:10.1051/0004-6361/201936567
Context. Supernova remnants are known to accelerate cosmic rays on account of their nonthermal emission of radio waves, X-rays, and gamma rays. Although there are many
Context. Supernova remnants are known to accelerate cosmic rays on account of their nonthermal emission of radio waves, X-rays, and gamma rays. Although there are many
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c62a7867539c907ed87ab0b86bb1884
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jul2021, Vol. 505 Issue 1, p755-770, 16p
Autor:
Petruk, Oleh, Kuzyo, T., Orlando, S., Pohl, Martin Karl Wilhelm (Prof. Dr.), Miceli, M., Bocchino, F., Beshley, V., Brose, Robert (Dr.)
We present very-high-resolution 1D MHD simulations of the late-stage supernova remnants (SNRs). In the post-adiabatic stage, the magnetic field has an important and significant dynamical effect on the shock dynamics, the flow structure, and hence the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______266::74aa6e6ec326b4747057166240ab2c2e
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/52125
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/52125