Infrared studies of CO chemisorption on a highly dispersed supported Os catalyst
A highly dispersed titania-supported Os catalyst was prepared by the ion-exchange method. FT-IR was used to study CO chemisorption on the reduced catalyst. The IR spectra revealed two strong bands at 2129 and 2055 cm/sup -1/ and a shoulder at ca. 1990 cm/sup -1/. The frequencies and shapes of the ba...
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Veröffentlicht in: | J. Phys. Chem.; (United States) 1987-11, Vol.91 (23), p.6013-6016 |
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Sprache: | eng |
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Zusammenfassung: | A highly dispersed titania-supported Os catalyst was prepared by the ion-exchange method. FT-IR was used to study CO chemisorption on the reduced catalyst. The IR spectra revealed two strong bands at 2129 and 2055 cm/sup -1/ and a shoulder at ca. 1990 cm/sup -1/. The frequencies and shapes of the bands are independent of the adsorption pressure, i.e., surface coverage. The band at 2129 cm/sup -1/ was desorbed at 350/sup 0/C, and the other two bands were desorbed at the same temperature, 400/sup 0/C. Results of isotope exchange between C/sup 16/O and C/sup 18/O suggest that the band at 2129 cm/sup -1/ could be from the surface tricarbonyl species, Os(CO)/sub 3/, and the other two bands are from the surface dicarbonyl species, Os(CO)/sub 2/. No bridged or linear carbonyl species was observed. By comparison with the osmium carbonyl clusters, the Os particle size is about ten atoms and the average coordination number is about 4.8. |
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ISSN: | 0022-3654 1541-5740 |
DOI: | 10.1021/j100307a039 |