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Fig. A.4

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Evaporation rate (upper panel), and distribution of KER at eV (lower left panel) and eV (lower right panel) of (C54H18)4 for various combinations of parameters and assumptions. Cpot is the parameter of the attractive term in the LJ potential. BS and BO are the B rotational constants of the sphere and oblate top, respectively. A and C refer to the first and last rotational constants of the oblate top, respectively. All results are normalised to kevap = 1010 s-1 at eV. This implies that all models lead to equal areas of KER distributions at 6 eV, but different ones at 3 eV. See text for details.

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