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See detailHydrodechlorination of 1,2-dichloroethane on Pd-Ag catalysts supported on tailored texture carbon xerogels
Job, Nathalie ULg; Heinrichs, Benoît ULg; Ferauche, Fabrice et al

in Catalysis Today (2005), 102

Porous carbon xerogels synthesized in a previous study were investigated as catalysts supports. The support chosen was a micro-mesoporous carbon xerogel obtained from the pyrolysis of a resorcinol ... [more ▼]

Porous carbon xerogels synthesized in a previous study were investigated as catalysts supports. The support chosen was a micro-mesoporous carbon xerogel obtained from the pyrolysis of a resorcinol-formaldehyde resin whose synthesis variables were fixed at suitable values. Palladium and silver were deposited on this tailored texture carbon by co-impregnation using a solution of palladium and silver nitrates in nitric acid and water. Several catalysts were prepared with various Pd and Ag global contents, the latters being measured experimentally. Alloy particles, detected in all bimetallic samples, were studied by a combination of various techniques that enabled us to obtain their size as well as their bulk and surface composition. When present, the fraction of unalloyed silver was also calculated. The characterization data were related to the results of catalytic tests obtained for selective hydrodechlorination of 1,2-dichloroethane into ethylene. Results show that when the Ag content is too high, pure Ag particles are formed and the alloy composition remains constant. As a consequence, the surface composition of the alloy is constant as well and the catalytic tests lead to similar results. (c) 2005 Elsevier B.V. All rights reserved. [less ▲]

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See detailHydrodechlorination of 1,2-dichloroethane on Pd-Ag catalysts supported on texture-tailored materials
Job, Nathalie ULg; Heinrichs, Benoît ULg; Ferauche, Fabrice et al

Conference (2004, July 19)

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See detailHydrodynamic and hydrodispersive behaviour of chalk under variably saturated conditions
Brouyère, Serge ULg

Conference (2003, March 11)

The presentation describes a conceptual and mathematical model for solute migration in variably saturated fractured dual porosity, dual permeability chalk

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See detailHydrodynamic and hydrodispersive behaviour of variably saturated chalk : a field investigation
Brouyère, Serge ULg

Conference (2003, March 19)

The presentation described field investigations on contaminant transport across unsaturated chalk rocks, including tracer tests

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See detailHydrodynamic Approaches to Design Balancing Ponds
Pirotton, Michel ULg

in Marshall, English; Andras, Szollosi-Nagy (Eds.) Managing Water: Coping with Scarcity and Abundance (1997)

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See detailHydrodynamic forces acting on vertically translating bodies in free surface water
Kerger, François ULg; Detrembleur, Sylvain ULg; Archambeau, Pierre ULg et al

in WIT Transactions on The Built Environment, Vol 105, Fluid Structure Interaction V (2009, May)

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See detailHydrodynamic modelling, damage evaluation and technical adaptation measures
Dewals, Benjamin ULg

Conference (2008, January 10)

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See detailHydrodynamic models of the West European Shelf
Djenidi, Salim ULg; Nihoul, Jacques ULg; Ronday, François ULg

in Phys. of Shallow Bays, Estuaries and Cont. Shelves (1986)

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See detailHydrodynamic simulations of galaxy formation
Thoul, Anne ULg

in Dark Matter (1995, July)

We have developed an accurate, one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photo-ionization on the formation of ... [more ▼]

We have developed an accurate, one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photo-ionization on the formation of protogalaxies. We examine the ability of collapsing perturbations to cool within the age of the universe. In contrast to some studies based on order-of-magnitude estimates, we find that cooling arguments alone cannot explain the sharp upper cutoff observed in the galaxy luminosity function. We also look at the effect of a photoionizing background on the formation of low-mass galaxies. [less ▲]

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See detailHYDRODYNAMIC SIMULATIONS OF GALAXY FORMATION .1. DISSIPATION AND THE MAXIMUM MASS OF GALAXIES
Thoul, Anne ULg; WEINBERG, D. H.

in Astrophysical Journal (1995), 442(2), 480-491

We describe an accurate, one-dimensional, spherically symmetric Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photoionization on the formation of ... [more ▼]

We describe an accurate, one-dimensional, spherically symmetric Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photoionization on the formation of protogalaxies. The code can treat an arbitrary number of fluid shells (representing baryons) and collisionless shells (representing cold dark matter). As a test of the code, we reproduce analytic solutions for the pulsation behavior of a poly-trope and for the self-similar collapse of a spherically symmetric, cosmological perturbation. In this paper we concentrate on the effects of radiative cooling, examining the ability of collapsing perturbations to cool within the age of the universe. In contrast to some studies based on order-of-magnitude estimates, we find that cooling arguments alone cannot explain the sharp upper cutoff observed in the galaxy luminosity function. [less ▲]

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See detailHydrodynamic simulations of galaxy formation .2. Photoionization and the formation of low-mass galaxies
Thoul, Anne ULg; Weinberg, D. H.

in Astrophysical Journal (1996), 465(2), 608-616

Photoionization by the high-redshift ultraviolet radiation background heats low- density gas before it falls into dark matter potential wells, and it eliminates the neutral hydrogen and singly ionized ... [more ▼]

Photoionization by the high-redshift ultraviolet radiation background heats low- density gas before it falls into dark matter potential wells, and it eliminates the neutral hydrogen and singly ionized helium that dominate cooling of primordial gas at temperatures of 10(4)-10(5) K. We investigate the influence of photoionization on galaxy formation using high-resolution simulations with a one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code. We find that the presence of a photoionizing background suppresses the formation of galaxies with circular velocities v(circ) less than or similar to 30 km s(-1) and substantially reduces the mass of cooled baryons in systems with circular velocities up to v(circ) similar to 50 km s(-1). Above v(circ) similar to 75 km s(-1), photoionization has no significant effect. Photoionization exerts its influence primarily by heating gas before collapse; the elimination of line cooling processes is less important. We discuss the implications of these results for hierarchical theories of galaxy formation. [less ▲]

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See detail"Hydrodynamic Stress of Cellulases in a Bioreactor"
Meurisse, E.; Evrard, J. F.; Denoo, O. et al

in Mededelingen - Faculteit Landbouwwetenschappen, Rijksuniversiteit Gent (1993), 58(4b), 1981-1983

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See detailHydrodynamic stress of Dunaliella tertiolecta.
Rikir, R.; Spoiden, J. F.; Thonart, Philippe ULg

Poster (1990, July)

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See detailHydrodynamic systems used to assess surface fouling, soil adherence and cleaning in laboratory installations.
Detry, J. G.; Deroanne, Claude; Sindic, Marianne ULg

in Biotechnologie, Agronomie, Société et Environnement = Biotechnology, Agronomy, Society and Environment [=BASE] (2009)

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See detailHydrodynamical and ecosystem modelling on an IBM SP/2
Beckers, Jean-Marie ULg; Grégoire, Marilaure ULg; Rixen, M.

in Procedings of the second annual MMARIE (1997)

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See detailHydrodynamical and ecosystem modelling on an IBM SP/2 (part II)
Elmoussaoui, A.; Grégoire, Marilaure ULg; Nomérange, P. et al

in Procedings of the third annual MMARIE meeting (1998)

Detailed reference viewed: 1 (1 ULg)