Zobrazeno 1 - 10
of 16
pro vyhledávání: '"P. E., Gladilin"'
Publikováno v:
Physics of Atomic Nuclei. 81:1350-1354
The origin of cosmic rays is one of the most important questions in modern astrophysics. Leading world observatories are engaged in their search in our Galaxy and beyond. Current observations of bright sources of hard X-rays and gamma radiation requi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72bb97143333cd079ab2260381b0db22
https://doi.org/10.1134/s1063778818090120
https://doi.org/10.1134/s1063778818090120
Publikováno v:
Bykov, A. M.; Ellison, D. C.; Gladilin, P. E.; Osipov, S. M. (2015). Ultrahard spectra of PeV neutrinos from supernovae in compact star clusters. Monthly notices of the Royal Astronomical Society, 453(1), pp. 113-121. Oxford University Press 10.1093/mnras/stv1606
Starburst regions with multiple powerful winds of young massive stars and supernova remnants are favorable sites for high-energy cosmic ray acceleration. A supernova shock colliding with a fast wind from a compact cluster of young stars allows the ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79a0d4426c559918bc911567a42c47da
https://doi.org/10.1093/mnras/stv1606
https://doi.org/10.1093/mnras/stv1606
Publikováno v:
Journal of Physics: Conference Series. 929:012014
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::75734ad18d867ac60f4dc0ae38244548
https://doi.org/10.1088/1742-6596/929/1/012014
https://doi.org/10.1088/1742-6596/929/1/012014
Publikováno v:
Journal of Physics: Conference Series. 929:012006
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2c35576f37b654d487b9d947e1afc21a
https://doi.org/10.1088/1742-6596/929/1/012006
https://doi.org/10.1088/1742-6596/929/1/012006
Publikováno v:
AIP Conference Proceedings; 2017, Vol. 1792 Issue 1, p1-10, 10p, 7 Graphs
Publikováno v:
Journal of Physics: Conference Series. 769:012010
The observed appearance of the high-energy gamma-ray emission from galactic star clusters is determined by the geometry of the cluster and the distribution of the energy sources inside the cluster. A large number of massive stars with strong winds an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f8834a74d48a69a36485b2ba89e6edb1
https://doi.org/10.1088/1742-6596/769/1/012010
https://doi.org/10.1088/1742-6596/769/1/012010
Powerful stellar winds and supernova explosions with intense energy release in the form of strong shock waves can convert a sizeable part of the kinetic energy release into energetic particles. The starforming regions are argued as a favorable site o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33207bfb0ed4435a8150201779630ec6
http://arxiv.org/abs/1212.1556
http://arxiv.org/abs/1212.1556
We discuss processes in galactic cosmic ray (GCR) acceleration sites - supernova remnants, compact associations of young massive stars, and superbubbles. Mechanisms of efficient conversion of the mechanical power of the outflows driven by supernova s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::284ef9d1d8f6dd84fc6c7c2846b7e4a8
Publikováno v:
Journal of Physics: Conference Series. 661:012004
We present the 2D axisymmetric model of particle acceleration at colliding shocks from supernova remnant and stellar wind from the nearby star. The model is the expansion of the previously developed plane-parallel model and takes into account three t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::969581162364012a89df81ed2a46347e
https://doi.org/10.1088/1742-6596/661/1/012004
https://doi.org/10.1088/1742-6596/661/1/012004
Publikováno v:
Journal of Physics: Conference Series. 572:012003
We have shown that maximal energies of the charged particles accelerated in the system of converging magnetohydrodynamic (MHD) flows can reach ≈ 1017 eV. The scheme of magnetic field amplification (MFA) applied to the previous non-linear model of p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c7708b0cabceddb13f4cd341f5d9d9bc
https://doi.org/10.1088/1742-6596/572/1/012003
https://doi.org/10.1088/1742-6596/572/1/012003