Search Results - "Kuzyo, T"

Post-adiabatic supernova remnants in an interstellar magnetic field: parallel and perpendicular shocks by Petruk, O., Kuzyo, T., Beshley, V.

“…Gamma-rays from hadronic collisions are expected from supernova remnants (SNRs) located near molecular clouds. The temperature of the shock interacting with…”
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Magneto-hydrodynamic simulations of young supernova remnants and their energy-conversion phase by Petruk, O, Kuzyo, T, Orlando, S, Pohl, M, Brose, R

“…ABSTRACT Supernova remnants (SNRs) can be rich sources of information on the parent SN (supernova) explosion. Thus, investigating the transition from the phase…”
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Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment by Petruk, O, Kuzyo, T, Orlando, S, Pohl, M, Miceli, M, Bocchino, F, Beshley, V, Brose, R

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Constraints on magnetic field strength in the remnant SN 1006 from its non-thermal images by Petruk, O., Kuzyo, T., Bocchino, F.

“…Images of SN 1006 have a number of important properties. For instance, the bright limbs coincide spatially in various bands, they have different brightnesses,…”
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Erratum: Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment by Petruk, O, Kuzyo, T, Orlando, S, Pohl, M, Miceli, M, Bocchino, F, Beshley, V, Brose, R

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Constraints on magnetic field strength in the remnant SN 1006 from its non-thermal images: Magnetic field and images of SN 1006 by Petruk, O., Kuzyo, T., Bocchino, F.

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Individual particle approach to the diffusive shock acceleration. Effect of the non-uniform flow velocity downstream of the shock by Petruk, O, Kuzyo, T

“…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…”
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Magneto-hydrodynamic simulations of young supernova remnants and their energy-conversion phase by Petruk, O, Kuzyo, T, Orlando, S, Pohl, M, Brose, R

“…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…”
Get full text

Post-adiabatic supernova remnants in the interstellar magnetic field. Parallel and perpendicular shocks by Petruk, O, Kuzyo, T, Beshley, V

“…Gamma-rays from hadronic collisions are expected from supernova remnants (SNRs) located near molecular clouds. The temperature on the shock interacting with…”
Get full text

Post-adiabatic supernova remnants in an interstellar magnetic field: oblique shocks and non-uniform environment by 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…”
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Constraints on magnetic field strength in the remnant SN1006 from its nonthermal images by Petruk, O, Kuzyo, T, Bocchino, F

“…Images of SN1006 have a number of important properties. For instance, the bright limbs coincide spatially in various bands, they have different brightness, and…”
Get full text