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. 2022 Sep 6;23(18):10264. doi: 10.3390/ijms231810264

Figure 4.

Figure 4

(a,b) Potential mean force (PMF) (in kcal/mol) as a function of SASA and RG of the hIAPP20–29 octamer and hIAPP20–29 + Mel systems in the absence and presence of Mel. (c,d) Representative conformations of the first ten most-populated clusters in the hIAPP20–29 and hIAPP20–29 + Mel systems. The corresponding percentage is given in parentheses.