Introduction to Stellar Astrophysics: Volume 3This book is the final one in a series of three texts which together provide a modern, complete and authoritative account of our present knowledge of the stars. It discusses the internal structure and the evolution of stars, and is completely self-contained. There is an emphasis on the basic physics governing stellar structure and the basic ideas on which our understanding of stellar structure is based. The book also provides a comprehensive discussion of stellar evolution. Careful comparison is made between theory and observation, and the author has thus provided a lucid and balanced introductory text for the student. As for volumes 1 and 2, volume 3 is self-contained and can be used as an independent textbook. The author has not only taught but has also published many original papers in this subject. Her clear and readable style should make this text a first choice for undergraduate and beginning graduate students taking courses in astronomy and particularly in stellar astrophysics. |
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Índice
II | 1 |
III | 11 |
IV | 13 |
V | 14 |
VI | 16 |
VII | 18 |
VIII | 20 |
IX | 21 |
LXIV | 142 |
LXV | 151 |
LXVI | 155 |
LXVII | 158 |
LXVIII | 164 |
LXIX | 168 |
LXX | 169 |
LXXI | 170 |
XI | 24 |
XII | 25 |
XIII | 29 |
XIV | 32 |
XV | 35 |
XVI | 38 |
XVII | 39 |
XVIII | 42 |
XX | 48 |
XXII | 51 |
XXV | 53 |
XXVI | 56 |
XXVII | 61 |
XXVIII | 64 |
XXIX | 67 |
XXX | 69 |
XXXI | 71 |
XXXII | 74 |
XXXIII | 76 |
XXXIV | 77 |
XXXV | 79 |
XXXVII | 81 |
XXXVIII | 83 |
XXXIX | 84 |
XL | 86 |
XLI | 87 |
XLII | 89 |
XLIII | 93 |
XLIV | 95 |
XLV | 96 |
XLVI | 97 |
XLVII | 98 |
XLVIII | 100 |
XLIX | 102 |
L | 106 |
LII | 107 |
LIII | 108 |
LIV | 109 |
LV | 113 |
LVI | 117 |
LVII | 121 |
LVIII | 126 |
LIX | 130 |
LX | 132 |
LXI | 136 |
LXII | 139 |
LXIII | 141 |
LXXII | 172 |
LXXIII | 176 |
LXXIV | 177 |
LXXV | 182 |
LXXVI | 186 |
LXXVII | 189 |
LXXVIII | 192 |
LXXIX | 197 |
LXXX | 198 |
LXXXI | 200 |
LXXXII | 202 |
LXXXIII | 203 |
LXXXVI | 206 |
LXXXVII | 211 |
LXXXVIII | 213 |
LXXXIX | 216 |
XC | 217 |
XCI | 220 |
XCII | 222 |
XCIII | 227 |
XCIV | 228 |
XCV | 229 |
XCVI | 231 |
XCVII | 235 |
XCVIII | 236 |
XCIX | 237 |
C | 238 |
CI | 239 |
CIII | 240 |
CIV | 242 |
CV | 243 |
CVI | 245 |
CVII | 246 |
CVIII | 248 |
CIX | 251 |
CX | 256 |
CXI | 257 |
CXII | 260 |
CXIII | 261 |
CXIV | 262 |
CXVI | 264 |
CXVII | 265 |
CXVIII | 266 |
CXIX | 273 |
280 | |
283 | |
Otras ediciones - Ver todo
Introduction to Stellar Astrophysics: Stellar structure and evolution E. Böhm-Vitense No hay ninguna vista previa disponible - 1992 |
Introduction to Stellar Astrophysics: Volume 3 Erika Böhm-Vitense No hay ninguna vista previa disponible - 1989 |
Términos y frases comunes
abundances adiabatic amount assumed atmosphere atom average becomes blue boundary branch bubble calculated called cent central Cepheids Chapter cloud clusters color compared constant contraction convection zone cool core decreases density depends depth derived determined diagram discussed distance distribution dwarfs electrons elements energy transport equation equilibrium estimate evolution expands expect factor flux follow forces function giant give given gravitational heat heavy helium higher hydrogen hydrostatic important increase instability interior ionization larger layer lower luminosity magnitude main sequence mass massive material means mixing neutrinos neutron nuclear observed obtain occurs particles position pressure proton-proton chain pulsation radiation radiative equilibrium radius reach reactions region relation shown smaller solar stars stellar stratification surface Teff temperature temperature gradient values velocity Volume wavelength
Pasajes populares
Página 281 - Stetson, PB, VandenBerg, DA, Bolte, M., Hesser, JE and Smith, GH 1989, Astron. J., 97, 1360.
Página 281 - Rosseland, S. 1949, The Pulsation Theory of Variable Stars , Clarendon Press, Oxford.
Página 281 - Chandrasekhar, S., An Introduction to the Study of Stellar Structure. University of Chicago Press, Chicago, 1939.