Asymmetric Drift And Rotation Curve From RAVE And SEGUE Data

Details Asymmetric Drift And Rotation Curve From RAVE And SEGUE Data Asymmetric Drift And Rotation Curve From RAVE And SEGUE Data

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21944504g&link_type=abstract

American Astronomical Society, AAS Meeting #219, #445.04

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Scientific paper

We use RAVE, SEGUE and Hipparcos data to study the asymmetric drift in the solar neighbourhood. We study the metallicity dependence of the asymmetric drift, discuss the reliability of the local standard of rest, and justify the asymmetric drift correction consistent with our data. SEGUE data are then used to trace the rotation curve of the Galaxy in the extended solar neighbourhood. Supplementing these data by other measurements of the rotation curve, we construct an improved mass model of the Milky Way.

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