Fig. 12

Relations between ξLyα, the “relative Petrosian extension of Lyα” as defined in Hayes et al. (2013), and global kinematical parameters vshear, σ0 and vshear/σ0 with symbols according to the legend in Fig. 9. For galaxies with no Lyα emission (LARS 4 and LARS 6, circled symbols) ξLyα is defined as zero and for LARS 9 the measured ξLyα presents a lower limit (see also Hayes et al. 2013). Spearman rank correlation coefficients ρs and corresponding p0 values are calculated excluding LARS 4 and LARS 6.
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