The local rotation curve of the Milky Way based on SEGUE and RAVE data
K. Sysoliatina (1), A. Just (1), O. Golubov (2,3,4), Q.A. Parker, (5,6), E.K. Grebel (1), G. Kordopatis (17), T. Zwitter (15), J., Bland-Hawthorn (14), B.K. Gibson (8), A. Kunder (16), U. Munari (7), J., Navarro (12), W. Reid (10,11), G. Seabroke (9), M.Steinmetz (18), and F.

TL;DR
This study constructs the Milky Way's rotation curve near the Sun using SEGUE and RAVE data, revealing a smooth curve without evidence of a massive overdensity ring outside the solar radius.
Contribution
It provides a new detailed analysis of the local rotation curve and disc kinematics using recent large survey data, challenging previous claims of overdensity features.
Findings
The rotation curve is smooth between 7-10 kpc from the Galactic center.
No evidence supports a massive overdensity ring outside the solar radius.
Derived the radial scalelengths for different stellar populations.
Abstract
We construct the rotation curve of the Milky Way in the extended solar neighbourhood using a sample of SEGUE (Sloan Extension for Galactic Understanding and Exploration) G-dwarfs. We investigate the rotation curve shape for the presence of any peculiarities just outside the solar radius as has been reported by some authors. We approach the problem in a framework of classical Jeans analysis. Using the most recent data from RAVE (RAdial Velocity Experiment), we determine the solar peculiar velocity and the radial scalelengths for the three populations of different metallicities representing the Galactic thin disc. Then with the same binning in metallicity for the SEGUE G-dwarfs, we construct the rotation curve in the range of Galactocentric distances 7-10 kpc. We derive the circular velocity by correcting the mean tangential velocity for the asymmetric drift in each distance bin. With…
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