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Direct observation of thermally activated NO adsorbate species on Au-TiO2: DRIFTS studies

Author
DEBEILA, M. A1 ; COVILLE, N. J1 ; SCURRELL, M. S1 ; HEARNE, G. R1
[1] Molecular Sciences Institute, School of Chemistry, Private Bag X3, University of the Witwatersrand, Johannesburg 2050, South Africa
Source

Journal of molecular catalysis. A, Chemical. 2004, Vol 219, Num 1, pp 131-141, 11 p ; ref : 80 ref

ISSN
1381-1169
Scientific domain
General chemistry, physical chemistry
Publisher
Elsevier, Amsterdam
Publication country
Netherlands
Document type
Article
Language
English
Author keyword
Adsorption Au-TiO2 DRIFTS NO Thermally stable
Keyword (fr)
Adsorption gaz solide Adsorption Azote monoxyde Catalyse hétérogène Catalyseur sur support Métal transition composé Or Spectrométrie IR Stabilité thermique Titane oxyde Spectrométrie DRIFT Métal transition
Keyword (en)
Gas solid adsorption Adsorption Nitric oxide Heterogeneous catalysis Supported catalyst Transition element compounds Gold Infrared spectrometry Thermal stability Titanium oxide Transition metal
Keyword (es)
Adsorción gas sólido Adsorción Nitrógeno monóxido Catálisis heterogénea Catalizador sobre soporte Oro Espectrometría IR Estabilidad térmica Titanio óxido Metal transición
Classification
Pascal
001 Exact sciences and technology / 001C Chemistry / 001C01 General and physical chemistry / 001C01A Theory of reactions, general kinetics. Catalysis. Nomenclature, chemical documentation, computer chemistry / 001C01A03 Catalysis

Pascal
001 Exact sciences and technology / 001C Chemistry / 001C01 General and physical chemistry / 001C01I Surface physical chemistry

Discipline
General chemistry and physical chemistry
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
15954675

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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