Stellar Physics: Stellar Evolution and StabilitySpringer Science & Business Media, 20/11/2001 - 383 من الصفحات "Stellar Physics" is a rather unique book in the growing literature on star formation and evolution. Not only does the author, a leading expert in the field, give a very thorough description of the current knowledge about stellar physics, but he handles with equal care the many problems that this field of research still faces. A bibliography with well over 650 entries makes this book an unparalleled source of references. "Stellar Evolution and Stability" is the second volume and can be read, as can the first volume, as a largely independent work. It traces in great detail the evolution of the protostar towards the main sequence and beyond this to the last stage of stellar evolution, with the corresponding vast range from white dwarfs to the mighty supernovae explosions and blackhole formation. The book concludes with special chapters on the dynamical, thermal and pulsing stability of stars. |
المحتوى
I | 1 |
II | 2 |
III | 5 |
V | 6 |
VI | 10 |
VII | 15 |
VIII | 16 |
IX | 18 |
LXIV | 175 |
LXVI | 177 |
LXVII | 179 |
LXVIII | 183 |
LXIX | 189 |
LXX | 193 |
LXXI | 194 |
LXXII | 199 |
X | 25 |
XIII | 28 |
XIV | 29 |
XV | 32 |
XVI | 33 |
XVII | 34 |
XVIII | 36 |
XIX | 39 |
XX | 44 |
XXI | 45 |
XXII | 49 |
XXIII | 54 |
XXIV | 58 |
XXV | 61 |
XXVII | 62 |
XXVIII | 63 |
XXIX | 64 |
XXXI | 65 |
XXXII | 66 |
XXXIII | 67 |
XXXIV | 74 |
XXXV | 76 |
XXXVI | 83 |
XXXVII | 95 |
XXXVIII | 103 |
XXXIX | 108 |
XLI | 110 |
XLII | 111 |
XLIII | 116 |
XLIV | 119 |
XLV | 121 |
XLVI | 128 |
XLVII | 131 |
XLVIII | 135 |
XLIX | 137 |
LI | 145 |
LII | 150 |
LIII | 151 |
LIV | 152 |
LV | 154 |
LVI | 156 |
LVII | 161 |
LVIII | 164 |
LIX | 165 |
LX | 168 |
LXI | 169 |
LXII | 170 |
LXIII | 174 |
LXXIII | 204 |
LXXV | 207 |
LXXVI | 209 |
LXXVII | 212 |
LXXVIII | 213 |
LXXIX | 216 |
LXXX | 220 |
LXXXI | 224 |
LXXXII | 225 |
LXXXIII | 226 |
LXXXV | 230 |
LXXXVI | 233 |
LXXXVII | 236 |
LXXXVIII | 261 |
LXXXIX | 263 |
XC | 265 |
XCI | 268 |
XCII | 272 |
XCIII | 274 |
XCIV | 276 |
XCV | 277 |
XCVI | 279 |
XCVII | 280 |
XCVIII | 283 |
XCIX | 284 |
C | 287 |
CI | 289 |
CII | 293 |
CIII | 294 |
CV | 296 |
CVI | 299 |
CVII | 301 |
CIX | 305 |
CX | 307 |
CXI | 309 |
CXII | 310 |
CXIII | 313 |
CXV | 315 |
CXVI | 316 |
CXVII | 317 |
CXVIII | 320 |
CXIX | 322 |
CXX | 325 |
CXXI | 365 |
CXXII | 377 |
379 | |
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عبارات ومصطلحات مألوفة
accretion accretion disk adiabatic angular momentum approximation AsJ Soviet Astronomy binary Bisnovatyi-Kogan black hole boundary carbon central density Chap coefficient collapse condition const convection core corresponding criterion curve degenerate disk electron emission entropy envelope equation equilibrium evolutionary calculations evolutionary tracks flash flux formation gravitational heat helium burning helium flash HR diagram hydrodynamical hydrogen increase initial lg Tef low-mass luminosity magnetic field main sequence mass loss massive stars matter maximum models neutrino neutron star nuclear nuclei observed obtain opacity oscillations outflow parameters phase transition planetary nebula polytropic pressure protostars pulsars pulsation radiation radiative radius reaction region rotating star Sect shell solar solution specific angular momentum stability stars with masses static stellar evolution stellar mass supernova supernova explosion Table Tauri stars temperature thermal instability viscosity white dwarf