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Fig. 11


Distribution of the inferred spin parameter proxy [λ × (jd/jDM)] computed from Eq. (1) for the subset of 23 rotation-dominated galaxies with a ratio V/σ> 1 (see Sect. 5.1.2). The red curve shows the theoretical lognormal P(λ) distribution for dark matter haloes with mean and dispersion σ = 0.57 (Bullock et al. 2001; Bett et al. 2007; Muñoz-Cuartas et al. 2011).

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