Open Access

Fig. 6.

image

Download original image

Ratio between the median SFR in the fiducial and non-AGN runs, across cosmic time, for our set of simulated dwarf galaxies, colour-coded by BH mass. In the left-hand panel, the ⟨SFR⟩AGN/⟨SFR⟩non−AGN ratio is shown against the z = 0 BH mass of each galaxy in the fiducial run, as a proxy for the total amount of energy available as AGN feedback. In the right-hand panel, this ratio is instead plotted against the BH mass over the stellar mass of the simulated galaxies: this relation shows much less scatter and a stronger correlation. The solid line and grey-shaded region show the best linear fit and the 1σ error of the sample, respectively.

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.