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Fig. 3


Value (31) of ρcrb for various halo masses (solid line). For the entire range of galactic masses (Mvir ≃ 109−1012 M) multiplication ρcrb remains almost constant. According to Eq. (22), ρcrb is inversely proportional to α. The dashed line represents ρcrb, if we use a lower value of α (Eq. (32) instead of (23)). This agrees well with observations (log (ρcrb) = 2.15 ± 0.2 in units of log (M pc-2)).

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