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Fig. 6.

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Global kinematical measures vs. stellar mass (left panels) and star-formation rate (from Hα; right panels) for the LARS (squares) and eLARS galaxies (circles). The left-hand top-, middle-, and bottom panels show vshear vs. M, σ vs. M, and vshear/σ0obs vs. M, respectively. The right-hand top-, middle-, and bottom panels, show vshear vs. SFRHα, σ 0 obs $ \sigma_0^\mathrm{obs} $ vs. SFRHα, and vshear/σ0obs vs. SFRHα. Rotating discs, perturbed rotators, and systems with complex kinematics are shown with purple, green, and orange symbols, respectively. Systems with double-component Hα profiles in some spaxels are shown with open symbols; these galaxies are not included in the calculation of Kendal’s τ and pτ for relations involving σ 0 obs $ \sigma_0^\mathrm{obs} $ and vshear/σobs.

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