Fig. B.5
Velocity profiles of the LMC. Rotation curve (vϕ), tangential velocity dispersion (σϕ), radial velocity (vR), and radial velocity dispersion (σR) from leftto right for each stellar evolutionary phase (from top to bottom). Velocities are in km s−1. Bottom row: result for the combined sample. The blue shaded areas correspond to the uncertainties.
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