NCR values of our sample of SN 1994W-like events. Comparisons include other main CCSN subtypes in a) NCR_Hα and b) NCR_NUV (Anderson et al. 2012; Habergham et al. 2014; Ransome et al. 2022, indicated in the legend as A12, H14, and R22, respectively). In c) NCR_Hα values of the SN 1994W-like sample are compared to those of a selection of massive stars in the LMC simulated at the distance of 60.1 Mpc based on the method and catalogues used by Kangas et al. (2017, indicated in the legend as K17). For RSGs, both the complete sample and a sub-sample of less massive RSGs with log(L/L_⊙)<4.6 are shown.