Editors' Foreword |
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xi | |
Preface to the English Edition |
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xiii | |
Preface to the First Russian Edition |
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xv | |
I. THE THEORY OF GRAVITATION |
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Einstein's Gravitational Equations |
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3 | (61) |
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The Equality of Inertial and Gravitational Mass |
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3 | (3) |
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The Fundamental Concept of the General Theory of Relativity |
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6 | (3) |
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Properties of Noninertial Systems |
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9 | (3) |
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The Measurement of Spacetime Intervals |
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12 | (4) |
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Some Formulae for Curvilinear Coordinates |
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16 | (3) |
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Dynamic and Kinematic Quantities |
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19 | (3) |
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22 | (2) |
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The Einstein Field Equations and the Equations of Motion |
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24 | (4) |
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The Cosmological Constant |
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28 | (5) |
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Newton's Law and Weak Gravitational Fields |
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33 | (4) |
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The Analogue of the Zeeman Effect in the Gravitational Field of a Rotating Body |
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37 | (1) |
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38 | (7) |
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Gravitational Radiation from Binary Stars |
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45 | (6) |
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Gravitational Radiation Damping |
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51 | (8) |
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The Detection of Gravitational Waves |
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59 | (5) |
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62 | (2) |
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Inescapability of the General Theory of Relativity (GTR) and Problems in the Theory of Gravitation |
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64 | (19) |
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64 | (1) |
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Unified Field Theory, Geometrodynamics, and the Fundamental Mass and Length |
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64 | (2) |
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A Flat-Space Theory of Gravity |
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66 | (2) |
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Necessity of the Concept of Spacetime Curvature |
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68 | (3) |
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On the Possibility of Calculating the Gravitation Constant from Elementary-Particle Theory |
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71 | (3) |
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74 | (4) |
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78 | (5) |
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80 | (3) |
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The Spherically Symmetric Gravitational Field |
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83 | (46) |
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83 | (2) |
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The Schwarzschild Gravitational Field |
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85 | (2) |
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The Gravitational Field inside a Star |
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87 | (2) |
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The Radial Motion of Light Rays and of Ultrarelativistic Particles |
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89 | (4) |
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Radial Motion of Nonrelativistic Particles |
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93 | (3) |
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Potential Curves for Nonradial Motion |
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96 | (3) |
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99 | (3) |
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The Motion of a Relativistic Particle in a Coulomb Field |
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102 | (1) |
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Gravitational Capture of a Nonrelativistic Particle |
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103 | (2) |
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Motion of Ultrarelativistic Particles and of Light Rays |
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105 | (1) |
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Particle Motion in the Schwarzschild Gravitational Field, including the Effects of Gravitational Radiation |
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106 | (4) |
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The R- and T-Regions of Schwarzschild Spacetime |
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110 | (5) |
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Internal Solution for a Nonstatic Sphere |
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115 | (3) |
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118 | (11) |
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Nonspherical Gravitational Fields |
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129 | (26) |
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129 | (1) |
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Static Fields with Axial Symmetry |
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130 | (4) |
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The External Fields of Rotating Bodies |
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134 | (4) |
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The Schwarzschild Sphere in an External Quadrupole Field |
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138 | (1) |
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The Gravitational Contraction of a Slowly Rotating Body with Small Deviations from Spherical Symmetry |
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139 | (5) |
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What Happens to Matter after It Falls through the Event Horizon? |
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144 | (11) |
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149 | (6) |
II. THE EQUATION OF STATE OF MATTER |
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155 | (5) |
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The Concept of Pressure; Different Kinds of Pressure; the Case of Long-Range Interactions |
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155 | (5) |
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160 | (41) |
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Classification into Domains |
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160 | (3) |
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163 | (4) |
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Corrections in the Domain of High Pressures |
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167 | (2) |
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The Domain of Medium Densities, 106 < ρ < 500 g cm-3 |
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169 | (5) |
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Nuclear Processes and Nuclear Interactions: Their Effect upon the Equation of State |
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174 | (7) |
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The Properties of a Neutron Gas |
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181 | (4) |
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Density Greater than Nuclear |
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185 | (2) |
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An Ideal Neutron Gas at Superhigh Density |
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187 | (1) |
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Ideal Gas with the Inclusion of Reciprocal Transformations between Particles |
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188 | (5) |
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Are All ``Elementary'' Particles Really Elementary? |
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193 | (1) |
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The Electromagnetic Interaction of Particles |
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194 | (3) |
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A Rigorous Limit upon the Equation of State? |
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197 | (4) |
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Properties of Matter at High Temperatures |
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201 | (10) |
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Physical Conditions in Ordinary Stars |
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201 | (1) |
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202 | (3) |
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Various Types of Equilibrium |
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205 | (6) |
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Thermodynamic Quantities at High Temperatures |
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211 | (22) |
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Neutral Gas, Plasma; Ionization Equilibrium |
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211 | (3) |
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The Thermodynamics of Radiation |
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214 | (3) |
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217 | (4) |
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The Dissociation of Nuclei |
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221 | (4) |
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Dense Matter at Low Temperatures |
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225 | (1) |
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226 | (2) |
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General Thermodynamic Relations for Truly Neutral Matter |
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228 | (5) |
III. RELATIVISTIC STAGES OF EVOLUTION OF COSMIC OBJECTS |
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233 | (6) |
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The Equilibrium and Stability of Stars |
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239 | (91) |
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The Equilibrium and Stability of a Star as a Whole |
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239 | (6) |
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General Aspects of the Theory of Stellar Equilibrium |
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245 | (4) |
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Analytic Theory of Polytropic Gas Spheres |
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249 | (3) |
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The Adiabatic and Polytropic Indices |
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252 | (2) |
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The Energy Approach to the Theory of Equilibrium for a Star Consisting of Matter with γ Close to 4/3 |
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254 | (2) |
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Relativistic Equations of Stellar Equilibrium |
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256 | (8) |
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Relativistic Equations for Rotating Stars |
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264 | (7) |
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Theory of Cold White Dwarfs |
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271 | (8) |
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279 | (7) |
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286 | (2) |
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Stability of Neutron Stars |
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288 | (3) |
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Configurations with Positive Energy |
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291 | (4) |
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The Metastability of Every Equilibrium State |
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295 | (2) |
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Equilibrium of a Supermassive Star |
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297 | (12) |
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Critical States of Stars with Intermediate Mass |
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309 | (21) |
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317 | (2) |
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319 | (3) |
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322 | (1) |
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322 | (3) |
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325 | (3) |
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328 | (2) |
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330 | (86) |
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Evolution of a Star up to the Loss of Stability or the White-Dwarf Stage |
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330 | (8) |
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Instability of Massive Stars with Nuclear Sources of Energy |
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338 | (2) |
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Stability of Stellar Evolution |
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340 | (5) |
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345 | (19) |
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The Physics of Neutron Stars |
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364 | (5) |
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Evolution of a Star with a Mass Greater than the Oppenheimer-Volkoff Limit |
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369 | (1) |
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370 | (3) |
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Neutrino Emission in the Collapse of a Cool Star |
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373 | (3) |
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The Evolution of a Supermassive Star: General Remarks |
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376 | (1) |
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377 | (2) |
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The Evolution of a Supermassive Star without Turbulence or Rotation |
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379 | (5) |
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Rotation and Mass Shedding: General Relationships |
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384 | (5) |
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Equilibrium and the Shape of a Rotating Star: The Newtonian Theory |
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389 | (4) |
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Corrections for GTR in the Theory of a Rotating Star |
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393 | (5) |
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Approximate Theory of Equilibrium |
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398 | (2) |
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Rotating Massive Stars and Quasistellar Objects |
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400 | (3) |
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403 | (2) |
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The Evolution of a Rotating Star: Velocity of Mass Ejection |
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405 | (11) |
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410 | (6) |
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416 | (16) |
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General Overview and Basic Equations |
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416 | (5) |
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Solutions for Nonrelativistic Star Clusters |
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421 | (3) |
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The Stability of Collisionless Solutions |
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424 | (2) |
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Physical Conditions, Collisions, and Evolution in Star Clusters |
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426 | (2) |
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Relativistic Star Clusters |
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428 | (4) |
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Physical Processes in the Vicinities of Relativistic Objects and a Comparison with Observations |
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432 | (41) |
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Accretion of Gas by Neutron Stars and Collapsed Stars |
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432 | (1) |
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The Infall of Noninteracting Particles |
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433 | (2) |
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Four Regimes of Hydrodynamical Flow in the Case of Spherical Symmetry |
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435 | (3) |
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The Case of Accretion and the Validity of the Hydrodynamical Approximation |
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438 | (4) |
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The Luminosity due to Symmetric Accretion onto Neutron Stars and White Dwarfs |
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442 | (2) |
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The Problem of Discovering Collapsed Stars |
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444 | (2) |
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The Case of Asymmetric Gas Flow |
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446 | (5) |
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Accretion as a Factor in Stellar Evolution |
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451 | (1) |
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The Electrostatic Field, Acceleration of Positrons during Accretion, and Gamma-Ray Emission |
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451 | (1) |
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452 | (5) |
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The Superfluidity and Superconductivity of Highly Compressed Matter, and Their Influence on the Behavior of Neutron Stars |
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457 | (2) |
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Magnetic and Magneohydrodynamic Phenomena in Collapsing Bodies |
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459 | (5) |
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The Statistics of Stars at the Endpoint of Stellar Evolution |
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464 | (9) |
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473 | (12) |
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Observed Properties of Quasistellar Objects |
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473 | (3) |
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Theories of Quasistellar Objects |
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476 | (9) |
References |
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485 | (26) |
Author Index |
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511 | (5) |
Subject Index |
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516 | |