Figure 3 from Rotation Curve of the Milky Way from Classical Cepheids

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Rotation Curve of the Milky Way from Classical Cepheids

Authors: Przemek Mróz, Andrzej Udalski, Dorota M. Skowron, Jan Skowron, Igor Soszyński, Paweł Pietrukowicz, Michał K. Szymański, Radosław Poleski, Szymon Kozłowski, and Krzysztof Ulaczyk

2019 The Astrophysical Journal Letters 870 L10.

Provider: AAS Journals

Caption: Figure 3.

Peculiar (noncircular) motions of Cepheids, after subtracting the model of Galactic rotation (model 2, linear rotation curve). U_s is the velocity component toward the Galactic center, V_s—along the Galactic rotation, and W_s toward the North Galactic pole.

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