Fig. 14

Download original image
Summary of some of the properties of the stellar haloes identified by ASOHF in the CAMELS, IllustrisTNG LH–1 simulation at z = 0. Left panel: distribution of half-mass radii. Middle panel: relation of stellar mass to DM halo mass. Diagonal lines correspond to constant stellar fractions. Right panel: relation of 3D velocity dispersion to stellar mass.
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.