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

### From inside the book

Results 1-3 of 83

Page 138

Of particular interest is the

Of particular interest is the

**ratio**of maximum shadow elevation to observer's elevation which is uniquely defined by Petterson's model , given his assumptions on viscosity . Figure 17 clearly implies that to produce a 7 orbit ( 12 day ...Page 222

A small + near the center is the c.m. The arrows on the error boxes point Tidirection to Earth orbital phase convention : 10.75 critical Roche surface for mass

A small + near the center is the c.m. The arrows on the error boxes point Tidirection to Earth orbital phase convention : 10.75 critical Roche surface for mass

**ratio**= 1.7 -0.5 0.25 HZ Her Her X - 1 cm 0 1 2 3 4 10'cm I division Fig .Page 227

These results are strongly dependent on the assumed mass

These results are strongly dependent on the assumed mass

**ratio**, but are essentially independent of the assumed X - ray beam shape or the visibility function used . Curves for R = 1.0 , 1.5 , 1.65 , 2.0 , 2.5 are shown in fig . 9 .### What people are saying - Write a review

We haven't found any reviews in the usual places.

### 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

### Other editions - View all

### 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