## Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |

### From inside the book

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Page 79

There are no very simple

enough to measure easily with current techniques . There are three other

observable

connection with ...

There are no very simple

**effects**predicted by this model that appear largeenough to measure easily with current techniques . There are three other

observable

**effects**that have been discussed with varying degrees of care inconnection with ...

Page 429

Thus the

the degeneracy

1 ) neutrino mean free paths including neutral - current

Thus the

**effect**of neutral currents on these cross - sections is small compared tothe degeneracy

**effects**mentioned above but ... Figure 31 shows a comparison of1 ) neutrino mean free paths including neutral - current

**effects**and degeneracy ...Page 802

Relativistic

Schwarzschild black holes where r , OG M / c ? ... For a Kerr metric , however ,

there are some

BARDEEN ...

Relativistic

**effects**. Relativistic**effects**are unimportant for disks aroundSchwarzschild black holes where r , OG M / c ? ... For a Kerr metric , however ,

there are some

**effects**which have potentially observable consequences . SeeBARDEEN ...

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### Contents

Why are the stars as they are? | 1 |

Krzeminskis StarCen | 5 |

The theory of degenerate configurations the limiting | 7 |

Copyright | |

64 other sections not shown

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### Common terms and phrases

absorption accretion amplitude analysis antenna approximation assumed Astrophys BAHCALL binary black hole calculated colors considered consistent core corresponding cycle Cyg X-1 density dependence detail detected detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate existence expected field Figure flux frequency function geometry give given gravitational gravitational collapse important increases indicated intensity interesting Journ less Lett light curve limit lines magnetic mass measurements motion Nature neutron star noise observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations pulse radiation radio range ratio region relative rotation scale sensitivity shown shows spectrum stellar stellar wind suggested surface temperature transducer values variable variations velocity X-ray sources