“…Although no definite conclusion can be drawn from the results of the current study regarding the type of species that gives rise to this pair of bands and, more specifically, the number of carbonyl groups involved, a careful review of the literature has led us to believe that a tricarbonyl species is formed. Previous studies that concluded the presence of such a species were conducted using a series of varying concentrations of 12 CO and 13 CO, and, hence, were able to discern peaks that would otherwise be overlapped by stronger neighboring bands. ,, In contrast, studies that concluded the presence of a dicarbonyl species were performed using only a single concentration of a 12 CO− 13 CO mixture and the poorly resolved spectra obtained may have led to false conclusions. , Furthermore, the positions of the bands are very similar to those observed for ruthenium tricarbonyl complexes having a stoichiometry Ru 2 (CO) 6 X 4 (where X is Cl, Br, or I), which exhibit strong absorbances at 2143−2128 and 2075−2069 cm -1 and a weak absorbance at 2015−2010 cm -1 . ,, The exact positions of these bands are dependent on the electronegativity of the halogen ligands, with a downshift observed with decreasing electronegativity. , In the case of supported Ru catalysts, the formation of the tricarbonyl species is believed to be the result of a CO-induced oxidative disruption process of finely dispersed Ru clusters with the participation of hydroxyl groups from the support, forming electron-deficient Ru n + ( n ranging between 1 and 3) sites with Y−O−Ru linkages (Y = Al, Si, or Ti). ,, …”