Past activity of Sgr A⋆ is unlikely to affect the local cosmic-ray spectrum up to the TeV regime

Open Access

Fig. 4.

Evolution of f_outflow as a function of time and for various parameters. The left panel presents the influence of the propagation model (i.e. either anisotropic or isotropic) for our 29 pc resolution, single-pulse run (s29pc). The right panel shows the influence of the intermittence of the source.

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