
Polyhedron p. 2975 - 2984 (1998)
Update date:2022-07-30
Topics:
Din, Avi Bar
Bergman, Brian
Rosenberg, Edward
Smith, Ryan
Dastru', Walter
Gobetto, Roberto
Milone, Luciano
Viale, Alessandra
The coordination of ammonia and of aliphatic amines (RNH2(R = Et, n-Bu, S-Bu, t-Bu, cyclohexyl) and Et2NH) to the electron deficient clusters Os3(CO)9(μ3-η2-C 9H6N) (μ-H) (1) and Os3(CO)9(μ3-η2-XC 9H5N)(μ-H) (X = 5-NH2, 4; 3-NH2, 5; 6-NH2, 6; 5-Br, 7; 5-CH3, 8) has been studied. The initially formed adducts of the amines with 1 gradually isomerize to give a mixture of two isomers whose ratio varies with the cluster, the solvent and the amine. Studies of the variation of the isomer ratio with temperature yield ΔH° and ΔS° values for the isomer equilibrium. The primary cause of the change in the isomer ratio is the variation in ΔS° which is rationalized as being due to solvation effects. The overall structure of the two isomers is assigned on the basis of NMR measurements to one where the amine occupies an axial position on the cluster and where the hydride and quinoline ring bridge different edges of the cluster. The equilibrium constant for amine complex formation is primarily determined by the steric bulk of the amine. The amine substituted complex 4 shows absolutely no tendency to coordinate amines and this is ascribed to relief of the electron deficiency at the metal core by the mesomeric effects of the para-amino group. The isomeric 5 and 6, however, do undergo coordination of amines at the metal core. The 5-methyl substituted complex 8 does not complex amine either. Compounds 1,4-8 all undergo simple protonation with both coordinating (CF3CO2H) and non-coordinating acids (HBF4) to give cationic dihydrido complexes whose solution structures are elucidated by NMR techniques. The chemistry of these electron deficient clusters is compared with related μ3-η2 imidoyl complexes and can be understood in terms of the Hammett equation, at least for protonation.
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Doi:10.1246/bcsj.71.2621
(1998)Doi:10.1021/ic9803098
(1998)Doi:10.1016/S0040-4039(98)01742-0
(1998)Doi:10.1007/s13738-016-1029-1
(2017)Doi:10.1021/jo981458a
(1998)Doi:10.1016/j.physb.2019.411804
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