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

### From inside the book

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Page 53

The two reflection effects do not significantly change the ratio of the two minima

or of the two maxima , and the additional optical light contributed by the

secondary and by the two reflections only imperceptibly changes the absolute

The two reflection effects do not significantly change the ratio of the two minima

or of the two maxima , and the additional optical light contributed by the

secondary and by the two reflections only imperceptibly changes the absolute

**value**of the ...Page 59

K are very strongly influenced by mass motions . c ) The

correspond to the larger

0.11 ...

**values**of Q. The smaller**values**of Q are acceptable only if the observed**values**ofK are very strongly influenced by mass motions . c ) The

**values**of M thatcorrespond to the larger

**values**of Q are lower than those of normal B 0.5 1 0.250.11 ...

Page 617

( Ez max = ( 1 + 2 / V3 ) ua ) , while remaining around our

1 and going to infinity at Ep ( ~ ( 3 ) * & ? ) . ... One , therefore , concludes that ( 52

) is indeed the proper limit one should take for Ez ma For «

( Ez max = ( 1 + 2 / V3 ) ua ) , while remaining around our

**value**in ( 52 ) for Ex ' >1 and going to infinity at Ep ( ~ ( 3 ) * & ? ) . ... One , therefore , concludes that ( 52

) is indeed the proper limit one should take for Ez ma For «

**values**which are not ...### What people are saying - Write a review

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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