“…The stability can usually be attributed to strong bonding between the interstitial, often a late transition metal, and a surrounding host metal from an early metal group, a circumstance that is another reminder of some early ideas of Brewer (1). Among the many reduced chalcogenides of the early transition metals that demonstrate these heterometal features are Ta M S (2, 3), Ta M Se (4), Ta MSe (5), Nb MS (6), Hf MTe (7), all with some combination of M"Fe, Co, Ni, Zr MTe (M"Mn, Fe, Co, Ni, Ru, Pt) (8), Hf MTe (9) (M"Mn}Fe), Nb Ni \V S >V (6), Ta MTe (M"Cr, Fe}Ni, Al, Si) (10,11), Sc Ni Te (12), Y M Te (M"Fe}Ni) (13), and Sc MTe (14) (M"Mn}Ni). Many of these phases also have a common structural motif, have tricapped trigonal prismatic clusters of the more active metal that share basal faces, and are centered by the late transition metal.…”