Figure 11.
The relation between subhalo mass fraction, fs, and the host halo's ‘dynamical age’, Nτ, defined as the number of dynamical time-scales elapsed since the formation of the (average) host halo (see equation 17). The left- and right-hand panels correspond to first- and second-order subhaloes, respectively. Symbols of different size and shades indicate different cosmologies. For each cosmology, there are five points, corresponding to the five halo masses, log (M0/ h− 1M⊙) = 11, 12, …, 15. The red lines are the best-fitting relations given by equations (19) and (20).

The relation between subhalo mass fraction, fs, and the host halo's ‘dynamical age’, Nτ, defined as the number of dynamical time-scales elapsed since the formation of the (average) host halo (see equation 17). The left- and right-hand panels correspond to first- and second-order subhaloes, respectively. Symbols of different size and shades indicate different cosmologies. For each cosmology, there are five points, corresponding to the five halo masses, log (M0/ h− 1M) = 11, 12, …, 15. The red lines are the best-fitting relations given by equations (19) and (20).

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