(a) Estimate dΘ/dR in the solar neighborhood, assuming that the Oort constants A and B are +14.8 and −12.4 km s−1 kpc, respectively. What does this say about the variation of Θ with R in the region near the Sun?
(b) If A and B were +13 and −13 km s−1 kpc, respectively, what would the value of dΘ/dR be? What would this say about the shape of the rotation curve in the solar neighborhood?