
Originally Posted by
kzb
The serious flaw with the original paper is said to be that the circular velocity is constant with z (perpendicular distance from the disc mid-plane).
Well, no. They said ...the mean azimuthal (or rotational) velocity of their tracer population is assumed to be independent of the Galactocentric cylindrical radius R at all heights. Which is "not supported by the data."
I'm no expert, but it appears to me that Moni Bidin, et al., just neglected to consider the asymmetric drift...
"The asymmetric drift is expected to vary with R, although this variation cannot be measured for [Moni Bidin's] sample as the data do not span a large enough range in R."
That also explains why Jo Bovy said:

Originally Posted by
kzb
"...the circular-speed curve of the Milky Way remains close to its value in the plane throughout the region |Z| < 4 kpc that we are investigating."
...which isn't a contradiction.