2015
DOI: 10.1016/j.cattod.2015.01.035
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Comparative study of the catalytic performance and final surface structure of Co3O4/La-CeO2 washcoated ceramic and metallic honeycomb monoliths

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Cited by 28 publications
(17 citation statements)
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“…Xie et al 757 found that preparation of a Co/AC catalyst in an air atmosphere promoted the formation of reactive oxygen species, leading to a high EA oxidation ability compared with the sample synthesized in nitrogen atmosphere. Gómez et al 758 and Hernández-Garrido et al 551 reported that Co/La-CeO2 was very active in the oxidation of EA, even more than the Pt/La-CeO2 catalyst.…”
Section: Ethyl Acetatementioning
confidence: 99%
“…Xie et al 757 found that preparation of a Co/AC catalyst in an air atmosphere promoted the formation of reactive oxygen species, leading to a high EA oxidation ability compared with the sample synthesized in nitrogen atmosphere. Gómez et al 758 and Hernández-Garrido et al 551 reported that Co/La-CeO2 was very active in the oxidation of EA, even more than the Pt/La-CeO2 catalyst.…”
Section: Ethyl Acetatementioning
confidence: 99%
“…However, the disadvantages of these catalysts, such as high cost, easypoisoning tendency and limited resources, hinder their wide industrial application. Alternatively, various transition metal oxides have been extensively studied over the past several years as oxidation catalysts because of their advantages including a lower price and adequate catalytic activities at relatively low temperature [3][4][5][6][7][8][9][10]. Among these metal oxides, Co 3 O 4 has attracted much attention due to its excellent catalytic performance in numerous reactions, e.g., the catalytic oxidation of CO, NO or VOCs as well as soot combustion [11][12][13][14][15][16][17][18].…”
Section: Introductionmentioning
confidence: 99%
“…Nevertheless, conventional SEM imaging does not provide information about the structure of the washcoating layer. To this end, an electron transparent cross-section of the monolith surface was prepared by FIB techniques and characterized by STEM, using High Angle-Annular Dark-Field mode (HAADF), Figure 2A,B, following the fruitful approach previously reported [13,14]. Figure 2A shows a low-mag view of the FIB cross-section (about 10 µm) of the monolith surface.…”
Section: Resultsmentioning
confidence: 99%