| Preface |
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xi | |
| Editors |
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xiii | |
| Contributors |
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xv | |
| Introduction |
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xvii | |
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Observational Evidence for Supermassive Black Holes |
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1 | (62) |
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1 | (4) |
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5 | (2) |
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7 | (4) |
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Resolved Stellar Dynamics |
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11 | (6) |
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Stellar Proper Motion Studies: The Galactic Center |
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11 | (3) |
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Integrated Stellar Dynamics |
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14 | (3) |
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Gas as a Tracer of the Gravitational Potential |
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17 | (7) |
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18 | (3) |
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HST Observations of Gas and Dust Disks |
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21 | (3) |
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Tackling the Unresolvable: Reverberation Mapping |
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24 | (9) |
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Observational Support as to the Reliability of Reverberation Mapping Masses |
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31 | (1) |
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Secondary Mass Estimators Based on Reverberation Mapping |
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32 | (1) |
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Scaling Relations for SMBHs |
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33 | (11) |
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33 | (2) |
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35 | (4) |
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Black Hole Masses and Light Concentration |
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39 | (2) |
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Black Hole Masses and Dark Matter Halos |
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41 | (3) |
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44 | (6) |
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50 | (13) |
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55 | (8) |
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Joint Evolution of Black Holes and Galaxies: Observational Issues |
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63 | (76) |
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Galaxy Activity: Generalities |
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64 | (1) |
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Local Evidence on the Interplay Between the Stellar and Gravitational Origin of AGN Activity |
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64 | (1) |
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The Starburst-AGN Connection |
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64 | (1) |
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The Missing Type-II AGN Population and Ultraluminous Infrared Galaxies |
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65 | (1) |
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The Cosmic History of Galaxy Activity |
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65 | (2) |
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Constraints on the Cosmic Energy Budget |
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67 | (1) |
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Obscured AGNs and Origin of the X-Ray Background |
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67 | (1) |
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The Cosmic IR Background: Contributions by AGNs and Starburst Galaxies |
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67 | (1) |
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Current Observational Programs and Future Perspectives |
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68 | (1) |
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Current Issues on Local Active Galaxies |
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68 | (20) |
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A Census of Local Active Galaxies |
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68 | (5) |
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The Missing Type-II AGN population |
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73 | (1) |
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IR Spectroscopy of Obscured Sources |
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74 | (4) |
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X-Ray Spectroscopy of ULIRGs |
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78 | (3) |
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An Evolutionary Sequence for Galaxy Activity |
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81 | (7) |
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Local Active Galaxies, Conclusions |
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88 | (1) |
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Faint Active Galaxies at High Redshifts: Overview |
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88 | (22) |
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High-Redshift Optical Quasars |
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89 | (6) |
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High-Redshift Radio Galaxies |
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95 | (3) |
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98 | (1) |
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Long-Wavelength IR and Millimetric Surveys |
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99 | (5) |
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Physics of the IR-Submillimeter Galaxy Population |
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104 | (5) |
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High-Redshift Active Galaxies: Conclusions |
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109 | (1) |
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Radiative and Baryonic Remnants of Past Activity |
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110 | (29) |
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The Cosmological Background Radiation |
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110 | (8) |
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Cosmological Evolutionary Patterns for AGNs |
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118 | (8) |
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Coeval Evolution of Starbursts and AGNs |
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126 | (2) |
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128 | (3) |
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Conclusions and Perspectives |
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131 | (2) |
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133 | (6) |
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Galaxy Formation in the Hierarchical Universe |
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139 | (68) |
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Formation and Evolution of Structure |
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141 | (9) |
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141 | (1) |
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The Primordial and Linear Power Spectra |
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142 | (5) |
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Linear Growth of Perturbations |
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147 | (1) |
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148 | (2) |
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The Formation of Dark Matter Halos |
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150 | (11) |
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The Spherical Tophat Collapse Model |
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150 | (3) |
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The Dark Matter Halo Mass Function: Press--Schechter |
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153 | (3) |
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The Conditional Halo Mass Function: Extended Press-Schechter |
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156 | (1) |
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156 | (2) |
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Agreement Between Semi-Analytic and N-Body Methods |
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158 | (3) |
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Spatial Clustering and Bias |
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161 | (4) |
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161 | (1) |
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162 | (3) |
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Dark Matter Halos: Internal Properties and Correlations |
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165 | (8) |
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165 | (2) |
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167 | (2) |
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Correlation Between Halo Properties and Formation History |
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169 | (4) |
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Galaxy Formation Within the CDM Paradigm |
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173 | (27) |
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Consumer's Guide to Galaxy Formation Models |
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173 | (2) |
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175 | (11) |
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Basic Predictions of CDM-Based Galaxy Formation Models |
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186 | (14) |
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200 | (7) |
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202 | (5) |
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Feedback in Cosmic Structures |
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207 | (32) |
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207 | (1) |
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208 | (6) |
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Closely Scale-Invariant DM |
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210 | (1) |
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Plasma in Hydrostatic Equilibrium |
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211 | (3) |
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214 | (2) |
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214 | (1) |
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215 | (1) |
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215 | (1) |
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216 | (6) |
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How Preheating Affects the Density Run |
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217 | (1) |
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How Preheating Changes the Boundary Condition |
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217 | (2) |
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The Overall Outcome, Hierarchical Preheating |
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219 | (3) |
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222 | (5) |
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External Preheating by AGNs |
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222 | (1) |
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Internal Impacts of Quasars |
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223 | (4) |
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Enhanced Sunyaev--Zel'dovich Effects |
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227 | (4) |
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Discussion and Conclusions |
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231 | (8) |
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235 | (4) |
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The Formation of Primordial Luminous Objects |
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239 | (52) |
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239 | (2) |
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241 | (12) |
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Fluctuations in the Early Universe |
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241 | (7) |
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From Fluctuations to Cosmological Structures |
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248 | (5) |
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Primordial Gas Properties |
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253 | (11) |
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253 | (1) |
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253 | (6) |
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259 | (5) |
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Numerical Cosmological Hydrodynamics |
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264 | (7) |
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Adaptive Refinement Codes (ENZO) |
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265 | (2) |
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Formation of the First Star |
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267 | (3) |
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270 | (1) |
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Protostar Formation and Accretion |
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271 | (7) |
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271 | (2) |
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273 | (5) |
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278 | (13) |
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279 | (3) |
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Supernovae Feedback and Metallicities |
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282 | (4) |
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286 | (5) |
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The Evolution of Baryons Along Cosmic History |
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291 | (34) |
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292 | (1) |
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The Dark Ages of the Universe |
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293 | (5) |
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Basic Physics of Recombination |
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293 | (1) |
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Post-Recombination Universe |
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294 | (3) |
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Linear Growth of Perturbations |
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297 | (1) |
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The Emergence of Cosmic Structures |
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298 | (3) |
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The Epoch of Reionization |
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301 | (8) |
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302 | (2) |
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Reionization by Massive Stars |
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304 | (2) |
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Reionization by Miniquasar |
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306 | (3) |
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Preheating and Galaxy Formation |
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309 | (3) |
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309 | (1) |
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310 | (2) |
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The Intergalactic Medium After Reionization |
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312 | (7) |
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Photoionization Equilibrium |
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313 | (2) |
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315 | (1) |
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316 | (3) |
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319 | (6) |
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321 | (4) |
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Feedback Processes at Cosmic Dawn |
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325 | (62) |
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326 | (4) |
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Hydrodynamics of Shock Waves |
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326 | (1) |
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Hydromagnetic Shock Waves |
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327 | (1) |
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328 | (2) |
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330 | (2) |
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332 | (3) |
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The Need for Feedback in Cosmology |
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335 | (12) |
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335 | (3) |
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Dwarf Galaxies: Feedback Lab |
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338 | (5) |
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Blowout, Blowaway and Galactic Fountains |
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343 | (2) |
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Further Model Improvements |
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345 | (2) |
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347 | (6) |
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Feedback as ISM Sterilization |
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347 | (4) |
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A Porosity-Regulated Feedback |
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351 | (1) |
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Advanced Multiphase/Feedback Schemes |
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352 | (1) |
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Feedback in the Early Universe |
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353 | (34) |
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355 | (6) |
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361 | (5) |
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Radiative Feedback and Reionization |
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366 | (18) |
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384 | (3) |
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The Ecology of Black Holes in Star Clusters |
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387 | (66) |
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387 | (20) |
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388 | (6) |
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394 | (2) |
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The Effect of Two-Body Relaxation: Dynamical Friction |
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396 | (2) |
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398 | (7) |
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405 | (2) |
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Theory of Star Cluster Evolution |
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407 | (10) |
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407 | (5) |
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Phase B: 10 Myr >~ t <~ 100 Myr |
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412 | (1) |
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413 | (2) |
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415 | (2) |
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Black Holes in Star Clusters |
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417 | (19) |
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The Formation of Intermediate Mass Black Holes in Phase A Clusters |
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418 | (5) |
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Calibration with N-Body Simulations |
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423 | (4) |
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Simulating the Star Cluster MGG11 |
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427 | (5) |
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Black Hole Ejection in Phase B and C Cluster with trt >~ 100 Myr |
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432 | (4) |
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Discussion and Further Speculations |
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436 | (10) |
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Turning an Intermediate Mass Black Hole in an X-Ray Source |
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436 | (1) |
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Speculation on the Formation of Supermassive Black Holes |
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437 | (1) |
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Is the Globular Cluster M15 a Special Case? |
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438 | (1) |
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The Gravitational Wave Signature of Dense Star Clusters |
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439 | (7) |
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446 | (7) |
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448 | (5) |
| Index |
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453 | |
Lisainfo e-raamatute kohta