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Fig. 9

image

Global Hα kinematical parameters vshear (left panel), σ0 (middle panel), and vshear/σ0 (right panel) in comparison to stellar mass for LARS galaxies (from Paper II) and in comparison to literature values: DYNAMO z ~ 0.1 [compact] perturbed rotators from Green et al. (2014) as [small] green circles; DYNAMO z ~ 0.1 [compact] complex kinematics from Green et al. (2014) as [small] green squares; Local Lyman Break Analogues from Gonçalves et al. (2010) as blue circles; Keck/OSIRIS resolved z ~ 2−3 star-forming galaxies from Law et al. (2009) as red circles; SINS z ~ 2−3 galaxies from Förster Schreiber et al. (2009) as orange squares (only in the left panel). Uncertainties given where available. The LARS galaxies are represented by symbols according to the legend in the left panel. Spearman rank correlation coefficients ρs and corresponding p0 values for the LARS galaxies are shown in each panel.

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