Comparison between the gas and dust mass-loss rates for our sample of uvAGBs. The colour and shape of the markers represent the stellar variability and chemistry type as in Fig. 4. Grey markers represent sources from the NESS sample. The dashed line represents the relationship presented in Wallström et al. (2025). The histograms at the top and to the right of the figure indicate the distribution of Ṁ_dust and Ṁ_gas respectively.