Part 1. Structure Formation Theory

Dynamical Approximations for Gravitational Clustering . . . . . . . . . 3
S. F. Shandardin
Optimizing Higher-Order Lagrangian Perturbation Theory for CDM Mod-
els . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13
A. G. Weiss, S. Gottlöber and T. Buchert
Gravitational Dynamics using the Deformation Tensor . . . . . . . . . . 19
E. Audit and J.-M. Alimi
Lagrangian Dynamics of Colfisioniess Matter . . . . . . . . . . . . . . . 25
S. Matarrese and D. Terranova
Cosmological Collapses of Irrotational Dust . . . . . . . . . . . . . . . . 31
M. Bruni
Modeffing the Clustering of Objects . . . . . . . . . . . . . . . . . . . . 37
E. Salvador-Solg
Tidal Fields and Structure Formation . . . . . . . . . . . . . . . . . . . 49
R. van de Weygaert
Evolution of the Angular Momentum of Protogalaxies from Tidal Torques 57
P. Catelan and T. Theuns
Gravitational Collapse in a Clumpy Environment . . . . . . . . . . . . . 63
V. Antonuccio-Delogu
The Structure Formation Resonance and its Time Evolution in a Quasi-
static Approximation . . . . . . . . . . . . . . . . . . . . . . . . . 69
P. G. Macedo and J. P. M. de Carvalho
Three Temperatures Hydrodynamics of Cosmological Pancakes . . . . . 75
R. Teyssier, J.-P. Chibze and J.-M. Alimi

Part 2. Numerical Methods and Results

Numerical and Analytical Studies of Galaxy Formation . . . . . . . . . 83
C. S. ftenk, C. M. Baugh and S. Cole
Modelling Generic Patches of the Universe . . . . . . . . . . . . . . . . . 95
E. Saar and L Suisalu
The Virgo Project: Cosmological Simulations using Hydra . . . . . . . . 101
P. A. Thornas, F. R. Pearce, H. M. P. Couchman, J. M. Colberg,
S. D. M. White, A. R. Jenkins and C. S. Frenk
Cosmic Structure on Small Scales: Results on Cluster Cores and Redshift-
Space Power Spectra . . . . . . . . . . . . . . . . . . . . . . . . . 107
B. C. Broinley, T. G. Brainerd, M. S. Warren and W. H. Zurek
A Hydrodynamic Cosmological Code: Preliminary Results . . . . . . . . 119
V. Quilis, J. M. Ibinez and D. Siez
Numerical Simulations of Galaxy Formation: Effects of Star Formation
and Gas Dynamics . . . . . . . . . . . . . . . . . . . . . . . . . . 125
G. Yepes, R. Kates, A. Klypin and A. Khokhlov
The Structure of Dark Matter Haloes . . . . . . . . . . . . . . . . . . . 131
G. Tormen
The Distribution of the Lya Absorption Clouds Tracing the Dark Matter
Filaments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 137
J. P. Micket

Part 3. Galaxy Redshift Surveys

Present and Future Redshift Surveys: ORS, DOGS and 2dF . . . . . . . 145
0. Lahav
Redshift Surveys and Large-Scale Structure . . . . . . . . . . . . . . . . 157
L. Guzzo
IRAS Galaxy Redshift Surveys . . . . . . . . . . . . . . . . . . . . . . . 171
M. Rowan-Robinson
Mapping the Universe through 3D Visualization of Galaxy Redshifts 177
L. L. Christensen
Large-Scale Structure at z - 2.5 . . . . . . . . . . . . . . . . . . . . . . 183
G. M. Williger, C. Hazard, J. A. Baldwin and R. G. McMahon

Part 4. Rich Galaxy Clusters

Projection Effects in the Abell Catalogue . . . . . . . . . . . . . . . . . 191
M. P van Haarlem
Galaxy Cluster Luminosity Functions and the Distances to Clusters 197
B. J. T. Jones and A. Mazure
Luminosity Function of Early-Type Galaxies in Cluster Cores (as selected
by ANN) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 205
E. Molinari and R. Smareglia
X-ray Selected Clusters of Galaxies . . . . . . . . . . . . . . . . . . . . 209
I. M. Gioia
Comparison of Optical and X-ray Structures of Galaxy Clusters . . . . 215
F. W. Baier, G. B. Lima Neto, H. Wipper and M. Braun
The Galaxy Velocity Dispersion - X-ray Temperature Relation in Galaxy
Clusters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 221
M. Girardi, D. Fadda, G. Giuricin, F. Mardirossian, M. Mezzetti and
A. Biviano

Part 5. Statistical Methods, Data Analysis and Tests of Models

The 2D Power Spectrum of Slices in the Las Campanas Redshift Survey:
Excesss Power and Quasi-Coherent Structures . . . . . . . . . . . 229
S. D. Landy
Laxge- and Superlarge-Scale Structure in the Universe: Core-Sampling
Approach . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 235
A. Doroshkevich and R. Fong
Multiscaling . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 241
V. J. Martinez and M. J. Pons-Borderia
Analyzing Galaxy Catalogues with Minkowski Functionals . . . . . . . . 247
M. Kerscher, J. Schmalzing and T. Buchert
The Statistics of the Large-Scale Velocity Field . . . . . . . . . . . . . . 253
F. Bernardeau
Redshift Space . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 259
A. F. Heavens
The Amplitude of the Initial Density Fluctuation Spectrum from Lensing
Statistics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 265
E. van Kampen
Do Galaxies of Different Characteristics Trace the Same Density Field? 271
R. Dominguez-Tenreiro
The Large-Scale Cluster Velocity Field and the Value of 9 . . . . . . . . 277
M, Plionis and E. Branchini
CDM like vs CIIDM Models: the Distribution of Galaxy Clusters . . . 283
S. Borgani
The Cluster Velocity Field . . . . . . . . . . . . . . . . . . . . . . . . . . 289
L. Moseardini, E. Branchini, P. Tini Brunozzi, S. Borgani, M. Plionis and
P. Coles
Cold + Volatile Dark Matter Models: L-.near Evolution and Large-Scale
Structure Predictions . . . . . . . . . . . . . . . . . . . . . . . . . 295
E. Pierpaoli
The Matter Distribution on CDM Models with Different Primordial
Perturbation Spectra . . . . . . . . . . . . . . . . . . . . . . . . . . . 301
S. GottliSber

Part 6. The Cosmic Microwave Background

What can we learn from CMB Anisotropies? . . . . . . . . . . . . . . . 309
N. Sugiyama
Non-linear Gravity and Anisotropies in the Cosmic Microwave Background
Radiation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 315
J. L. Sanz aijd L. Cayón
On the Microwave Background Anisotropy produced by Great Cosmolog-
ical Structures . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 325
M. J. Fullana, D. Sáez and J. V. Arnua
Is Tenerife Sampling an Active Region of the CBR Temperature
Fluctuation Sky . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 329
F. Atrio-Barandela and L. Cayón
Global Textures and the Doppler Peaks . . . . . . . . . . . . . . . . . . 335
A. Gangui, R. Durrer and M. Sakellariadou
Contributions to the GMBR Three-Point Function from the Rees-Sciama
Effect . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 341
S. Mollcrach, A. Gangui, F. Lucchin and 5. Mattarese

Part 7. Cosmological Models and Parameters

Averaging Hypotheses in Newtonian Cosmology . . . . . . . . . . . . . 349
T. Buchert
Cepheids, Supernovae and the Value of Ho . . . . . . . . . . . . . . . . 357
M. A. Hendry and S. M. Kanbur
Minimal Information and the Flatness Problem . . . . . . . . . . . . . . 363
P. Coles and G. Evrard
Modelling the Number Counts . . . . . . . . . . . . . . . . . . . . . . . 369
A. Campos
Can the Dark Matter be Fully Baryonic? . . . . . . . . . . . . . . . . . 375
J. M. Alimi and A. Serna

Author index . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 381