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

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Page 52

A systematie search for

revealed that a variety of

compared to values of M , ~ 14 M given by previous workers [ 8 , 23 - 25 ] .

A systematie search for

**solutions**based on these data by Avni and Bahcall [ 22 ]revealed that a variety of

**solutions**exists with a lower limit to M , of 8 . 5 Mo , ascompared to values of M , ~ 14 M given by previous workers [ 8 , 23 - 25 ] .

Page 342

This process was a consequence , KLEIN stressed , of the existence of

positiveand negative - energy states in the

. The understanding of this process was greatly deepened by the work of Sauter [

184 ] ...

This process was a consequence , KLEIN stressed , of the existence of

positiveand negative - energy states in the

**solutions**of relativistic wave equations. The understanding of this process was greatly deepened by the work of Sauter [

184 ] ...

Page 625

Concerning a more mathematical problem , the TS

some

the TS metric but also the other new metrics . A brief summary of the metric ...

Concerning a more mathematical problem , the TS

**solution**can be used to derivesome

**solutions**of the Einstein - Maxwell equation , not only a charged version ofthe TS metric but also the other new metrics . A brief summary of the metric ...

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### Contents

Gruppo fotografico del partecipanti al Corso | 1 |

Introduction | 17 |

Сen | 37 |

Copyright | |

59 other sections not shown

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### Common terms and phrases

absorption accretion amplitude analysis angular approximation assumed Astrophys binary black hole calculations charge considered convective core corresponding cycle density dependence detailed detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate evolution existence expected field Figure flux frequency function geometry give given gravitational important increase indicated intensity interesting Journ less Lett light curve limit lines magnetic mass mean measurements motion Nature neutrino neutron star observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations radiation radio range ratio region relation relative rotating scale sensitivity shell shown shows solutions spectrum stellar stellar wind structure suggested surface temperature values variable variations velocity X-ray sources