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Fig. 7


Rotation speed derived from Eq. (8) as a function of R for different z, with Δz = 400 pc; correction of systematic errors of proper motions included; adopting a solar azimuthal speed of Vg, ⊙ = 200 km s-1 and an LSR azimuthal speed of Vc(R,z = 0) = 188 km s-1. Error bars include statistical errors, uncertainties in (U,Vg, ⊙,W), and errors of the systematic errors of proper motion and contamination of non-RCGs.

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