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Vertical Structure, figures



FIGURE. 3.—Velocity allipcoid parameters as functions of heigt above the Galactic disk for the complete sample of F-stars (left) and a young (t&menrov;3 Gyr) metal-rich ([Fe/H]&menrov;-0.13) group (reght). The curves give σ1, σ2, and σ3 - the major, mean, and minor semi-axes of the ellipsoids, respectively; σ2/σ1 is the velocity ellipsoid semi-axis ratio; l&sun; is the Solar apex galactic longitude; L1 is the longitude component of the vertex deviation; v, u, and w are the components of the space velocity of the group centroids with respect to the Sun - the axes are directed toward the Galactic center (u>), in the direction of the Galactic rotation (v), and toward the North Galactic pole (w).
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