Open Access

Fig. 5.


Angular power spectrum for four models of the scaling of the magnetic field with the halo masses: (i) B0 = const. in solid red; (ii) an increase of the magnetic field for galaxies, i.e. at masses lower than 1013 M as given by Eq. (15) (dashed blue); and a combination of increased magnetic field for galaxies, Eq. (15), with a power law for massive clusters, Eq. (14), where (iii) γ = 0.25 (dotted green), and (iv) γ = 1 (dash-dotted orange).

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.