Fig. 4
Asymmetric drift for different data sets. The two black circles on the ΔV axis correspond to the different LSRs with V⊙ = 5.25 km s-1 from Aumer & Binney (2009) and V⊙ = 12.24 km s-1 from Schönrich et al. (2010) respectively. The grey line gives the best fit to the data points for RAVE dwarfs. It corresponds to the LSR V⊙ = −1.04 km s-1 and the scalelength of the disc Rd = 1.65 kpc.
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