Time-dependent galactic winds driven by cosmic ray advection and diffusion

Physics

Scientific paper

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Scientific paper

Numerical solutions are discussed for a time-dependent galactic wind
driven by advection and diffusion of cosmic rays. In this paper we
present the time-asymptotic solutions characterized by different
diffusion coefficients ( = 1027 , 1030 cm s,1 ) but having the same
cosmic rays flux at the inner boundary.

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