arXiv · astro-ph/9710055
The Shape and Scale of Galactic Rotation from Cepheid Kinematics
Abstract
A catalog of Cepheid variables is used to probe the kinematics of the Galactic disk. Radial velocities are measured for eight distant Cepheids toward l = 300; these new Cepheids provide a particularly good constraint on the distance to the Galactic center, R_0. We model the disk with both an axisymmetric rotation curve and one with a weak elliptical component, and find evidence for an ellipticity of 0.043 +/- 0.016 near the Sun. Using these models, we derive R_0 = 7.66 +/- 0.32 kpc and v_circ = 237 +/- 12 km/s. The distance to the Galactic center agrees well with recent determinations from the distribution of RR Lyrae variables, and disfavors most models with large ellipticities at the solar orbit.
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Mark R. Metzger, John A. R. Caldwell, Paul L. Schechter. 1997-10-06. The Shape and Scale of Galactic Rotation from Cepheid Kinematics. https://doi.org/10.1086/300198
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