Rendiconti della Scuola internazionale di fisica "Enrico Fermi."Academic Press, 1978 - Nuclear physics |
Contents
Why are the stars as they are? | 1 |
The theory of degenerate configurations the limiting | 7 |
Introduction | 17 |
Sanduleak 160SMC | 23 |
Color analysis | 24 |
Cen | 30 |
Cyg | 37 |
Introduction | 43 |
Introduction | 356 |
B M BARKER and R F OCONNELL Generalrelativistic | 437 |
43 | 442 |
Astrophysical applications | 472 |
Appendix A Pulsar Neutron stars Supernova explosion | 518 |
Appendix | 524 |
S A COLGATE | 539 |
T DAMOUR | 547 |
Applications | 52 |
The standard picture | 60 |
J N BAHCALL Optical properties of binary Xray sources | 63 |
Cygnus X1HDE 226868 | 71 |
Hz HerculisHer | 84 |
Optical pulsation | 90 |
Optical clues to the nature of accretion | 123 |
The accretion disk | 131 |
Confronting the Xray data | 139 |
Epilog | 146 |
Slow Xray pulsars | 156 |
R P GIFFARD S P BOUGHN W M FAIRBANK M | 166 |
StanfordLouisiana StateRome project | 173 |
HJELLMING Radioemission from compact Xray | 185 |
Cyg X3 the nanoquasar | 191 |
The energies and magnetic fields in radioemitting Xray | 198 |
J MIDDLEDITCH and J NELSON Optical pulsations from | 216 |
Elementary binary kinematics and variables | 222 |
Conclusions | 228 |
Introduction pag | 230 |
Centaurus X3 | 236 |
Cygnus X1 | 243 |
B STRONG Neutron stars black holes and gammaray | 250 |
H TANANBAUM Recent observations from Uhuru and ANS | 256 |
82 | 264 |
R RUFFINI Physics outside the horizon of a black hole | 287 |
83 | 299 |
ARNETT The final stages of the evolution of single | 349 |
H OKAMURA | 562 |
Introduction pag | 583 |
Numerical results | 590 |
T PIRAN and J SHAHAM Collisions in blackhole ergo | 597 |
Astrophysical layouts | 615 |
Conclusion | 622 |
Naked ring singularity and event horizon | 628 |
S TSURUTA Cooling and heating of neutron stars Current | 631 |
With accretion | 639 |
Equations | 646 |
Results for equilibrium configurations | 652 |
Results of dynamic calculations | 663 |
Appendix Nonaxisymmetric instabilities | 673 |
R A SUNYAEV Theory of accretion | 697 |
What do we see? | 706 |
Accretion of the stellar wind | 743 |
531 | 763 |
G BÖRNER F MEYER H U SCHMIDT and H C THOMAS | 764 |
FUJIMOTO and T MURAI An interpretation of the phe | 771 |
Flare stars | 780 |
Introduction | 786 |
Accretion onto neutron stars | 816 |
Accretion onto white dwarfs | 824 |
Evolution of single stars during hydrogen and helium | 831 |
Nonconservative evolution of close binaries | 857 |
95 | 862 |
Discussion rareness of the formation of systems like | 863 |
Copyright | |