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xi | |
Preface |
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xiii | |
Part one: Introduction to structure formation |
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1 | (75) |
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Dark matter and structure formation |
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3 | (73) |
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3 | (4) |
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7 | (5) |
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Age, expansion rate, and cosmological constant |
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12 | (11) |
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23 | (10) |
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33 | (9) |
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Origin of fluctuations: inflation and topological defects |
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42 | (12) |
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Comparing DM models to observations: ACDM vs. CHDM |
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54 | (22) |
References |
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76 | (21) |
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Gravitational instability |
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86 | (11) |
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86 | (2) |
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Linear theory and Zel'dovich approximation |
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88 | (2) |
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Nonlinear methods and mixed boundary conditions |
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90 | (7) |
References |
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97 | (34) |
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Microwave background and structure formation |
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98 | (33) |
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98 | (1) |
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Gravitational instabilities: linear theory |
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99 | (6) |
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105 | (6) |
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Galaxy formation by reverse engineering |
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111 | (7) |
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Cosmic microwave background anisotropies |
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118 | (5) |
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Confrontation of theory and large-scale structure |
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123 | (3) |
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126 | (5) |
References |
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131 | (38) |
Part two: Large-scale structure and flows |
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133 | (36) |
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Clusters and superclusters of galaxies |
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135 | (34) |
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135 | (1) |
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Optical properties of galaxy clusters |
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136 | (7) |
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X-ray properties of galaxy clusters |
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143 | (8) |
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The baryon fraction in clusters |
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151 | (1) |
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152 | (3) |
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Where is the dark matter? |
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155 | (1) |
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The mass function of clusters |
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155 | (1) |
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Quasar-cluster association |
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156 | (2) |
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158 | (2) |
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The cluster correlation function |
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160 | (4) |
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Peculiar motions of clusters |
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164 | (3) |
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167 | (2) |
References |
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169 | (39) |
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Redshift surveys of the local universe |
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172 | (36) |
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172 | (1) |
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Varieties of redshift surveys |
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173 | (5) |
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The luminosity and selection function |
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178 | (3) |
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181 | (3) |
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Measurements of the power spectrum |
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184 | (11) |
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The relative distribution of galaxies and dark matter |
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195 | (3) |
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198 | (8) |
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206 | (2) |
References |
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208 | (39) |
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Measurement of galaxy distances |
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213 | (1) |
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213 | (3) |
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216 | (3) |
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The Tully-Fisher relation for spiral galaxies |
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219 | (6) |
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Fundamental Plane relations for elliptical galaxies |
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225 | (4) |
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Surface brightness fluctuations |
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229 | (4) |
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233 | (4) |
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Brightest cluster galaxies |
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237 | (2) |
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Redshift-distance catalogs |
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239 | (2) |
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Malmquist and other biases |
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241 | (4) |
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245 | (2) |
References |
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247 | (68) |
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Large-scale flows and cosmological implications |
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250 | (65) |
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250 | (3) |
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Reconstruction from peculiar velocities |
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253 | (20) |
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273 | (7) |
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Statistics of mass-density fluctuations |
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280 | (9) |
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Direct measurements of Ω from peculiar velocities |
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289 | (4) |
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Measurements of β from galaxy density and velocities |
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293 | (13) |
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306 | (6) |
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312 | (3) |
References |
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315 | (20) |
Part three: Structure on galactic scales and lensing |
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319 | (16) |
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321 | (14) |
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321 | (2) |
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323 | (7) |
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Results: comparison with observations |
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330 | (2) |
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332 | (3) |
References |
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335 | (23) |
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Black holes in galaxy centers |
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337 | (21) |
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337 | (2) |
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Surface-brightness and stellar distributions |
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339 | (6) |
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Kinematic evidence for central massive black holes |
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345 | (13) |
References |
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358 | (68) |
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360 | (66) |
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360 | (4) |
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Lensing by point masses in the universe |
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364 | (20) |
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384 | (22) |
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Lensing by galaxy clusters and large-scale structure |
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406 | (20) |
References |
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426 | (38) |
Part four: A conclusion |
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433 | (31) |
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435 | (29) |
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435 | (8) |
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Dynamical mass measurements |
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443 | (12) |
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455 | (5) |
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460 | (3) |
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463 | (1) |
References |
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464 | (2) |
Index |
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466 | |