| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5422932 | Surface Science | 2011 | 10 Pages |
Abstract
⺠HT CO-desorption from TiO2 + Rh + COsat corresponds to C+O reaction on the titania support. ⺠Lack of CO2 suggests that O atoms arising from CO bind to reduced centers of titania. ⺠Preformed Mo particles increase the dispersion of rhodium deposit. ⺠Extended CO dissociation on Mo-Rh particles stems mainly from reaction with Mo. ⺠The Mo2C formed is a possible source of enhanced catalytic activity of Mo-Rh clusters.
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Authors
László Bugyi, Róbert Németh,