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Home All issues Volume 619 (November 2018) A&A, 619 (2018) A89 Full HTML
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Fig. 8.

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Top panel: mean log(MHI/Lr) ratio for NIBLES detections in each 0.5 dex wide luminosity bin, with uncertainties given by the standard error of the mean. The straight line indicates the least squares fit to the mean values. Middle panel: standard deviation (σ) of the log(MHI/Lr) ratio. Bottom panel: skewness of the log(MHI/Lr) ratio. All panels are a function of log(Lr) in L⊙.

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