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• W2002624850 abstract "Diffusive shock acceleration of energetic particles in a system of numerous stellar wind termination shocks and stellar-wind/supernova blast wave shocks is considered. We derive equations for the particle distribution function on momentum that describes collective particle acceleration. The form of the steady-state spectrum of accelerated particles depends on the global pattern of the interstellar gas flow. These results are discussed within a context of cosmic ray acceleration in star associations and in connection with a problem of cosmic ray reacceleration in the galactic disk." @default.
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• W2002624850 date "2000-05-01" @default.
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• W2002624850 title "Cosmic ray acceleration by multiple spherical shocks" @default.
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• W2002624850 doi "https://doi.org/10.1016/s0927-6505(99)00108-5" @default.
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