HESS J1745−290 spectrum explained by a transition in the diffusion regime of PeV cosmic rays in the Sgr A* accretion flow

Open Access

Fig. 6.

Gamma-ray spectrum for different maximum energies E_max = 1, 3, and 10 PeV (Cases 11, 2, and 12, respectively), all with the same parameter values n = 1, m = 0, q = 2, $\hat{B} = 1$ $\hat{B}=1$ , ${\hat{l}}_{c} = 3$ $\hat{l}_c=3$ , and slightly different values of $\hat{Q}$ $\hat{Q}$ , chosen so that the three spectra visually fit the H.E.S.S. data.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.