Eccentricity distribution (left panel) and mass ratio distribution (right panel) of the outer bodies in triples including Cepheids. The distribution for all triples (i.e. in star clusters and in the field combined) and the triples in the field and clusters only is shown by the yellow, black and cyan lines, respectively. We note that both distributions are remarkably different from the distributions of Cepheids in binaries, which are shown in Fig. 9.