Titlebook: Astrophysical Sources of High Energy Particles and Radiation; Maurice M. Shapiro,Todor Stanev,John P. Wefel Book 2001 Springer Science+Bus

allergen

Two-way ASP.NET/Flash Communication,different values of proton-proton cross sections are used. New results obtained recently in accelerator experiments lead to the necessity of revising some of them. In this paper, we show some results obtained in a framework of a so-called geometrical model. A particular proton profile function and i

hematuria

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Bricklayer

MAOIS

雪白

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https://doi.org/10.1007/978-1-4302-0103-8lectrons are accelerated on SNR shocks up to the energy ~ 10. eV. We have no direct observational confirmations about proton acceleration by SNR. Different models of γ-emission from SNRs predict different emission mechanisms as dominating. Only π° decays created in proton-nucleon interactions allow

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https://doi.org/10.1007/978-1-4302-0103-8scuss stochastic period evolution of INSs. We briefly discuss how an INS’s spin period evolves under influence of interaction with turbulized interstellar medium..To investigate statistical properties of the INS population we calculate a . of INSs in our Galaxy. We infer a lower bound for the mean k

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https://doi.org/10.1007/978-1-4302-0103-8utburst amounted to ~ 1.4 * 10. erg/sec, the same order of magnitudes as the luminosity of the ’giant’ X-ray outburst of the system. Probably, the flashes were even more powerful and more transient. These superfast and superpower processes could arise in the transient accretion disk of the pulsar wi

resilience

Two-way ASP.NET/Flash Communication,many attempts to explain them I focus here on the by now classical suggestion, that they come from powerful radio galaxies. In this review I will embed the discussion into a general framework of hadronic particle acceleration in Active galactic Nuclei.