The results of nuclear magnetic hfs alignment experiments on Ce 139 are presented, and are discussed in relation to those previously obtained for Ce 141 and Nd M7 . It is shown that the gamma-ray anisotropics, e, in the case of Ce 139 are consistent with a decay sequence 3/2 + ->5/2 + ->7/2 + , the gamma transition being Ml with ~4% admixture of E2. Even such a small admixture of E2 has an important effect upon the anisotropy through the interference term. Other factors which might affect the anisotropy are discussed: electron spin-spin interactions are important, whereas reorientation effects due to long lifetimes in the intermediate state are not. Interference is also important in the case of the 92-kev gamma ray following the decay of Nd 147 , where ^3% admixture of E2 radiation is needed to explain our results. It seems likely also that there is a similar effect in the 142-kev gamma ray following the decay of Ce 141 . The similarity of these mixtures (same magnitude and phase 4>=0) may not be fortuitous, since in each case the gamma ray connects levels which are classified by the shell model as dm and g 7 /2. In the cases of Ce 141 and Nd 147 the g 7 /2 state lies uppermost and e is reduced by the E2 admixture, whereas e is increased in Ce 139 , where the levels are inverted.