A detailed computational investigation of orbital interactions in metal-carbon bonds of metallyleneisocyanide adducts of the type R2MCNR´ (M = Si, Ge, Sn; R, R´ = alkyl, aryl) was performed using density functional theory and different theoretical methods based on energy decomposition analysis.Similar analyses have not been carried out before for metal complexes of isocyanides even though they have for long been of common practice when investigating the metal-carbon bonds in related carbonyl complexes. The results of our work reveal that the relative importance of -type backbonding interactions in these systems increases in the sequence Sn < Ge << Si and, in contrast to some earlier assumptions, the -component cannot be neglected for any of the systems investigated.While the fundamental ligand properties of isocyanides are very similar to those of carbonyl, there are significant variations in the magnitude of different effects observed. Most notably, when coordinated to metals, both ligands can display positive or negative shifts in their characteristic stretching frequency. However, because isocyanides are stronger -donors, the metal-induced changes in the CN bonding framework are greater than that observed for carbonyl. Consequently, isocyanides readily exhibit positive CN stretching frequency shifts even in complexes where they function as -acceptors, and the sign of these shifts is alone a poor indicator of the nature of the metal-carbon interaction. On the other hand, the relative -character of the metal-carbon bond in metallylene-isocyanide adducts, as judged by the natural orbitals of chemical valence as well as by partitioning the orbital interaction energy, was shown to have linear correlation with the shift in CN stretching frequency upon complex formation. The details of this correlation show that -back-[2] donation contributions need to exceed 100 kJ mol 1 in order for the shift in the CN stretching frequency of metallylene-isocyanide adducts to be negative.