## 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

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 or ~ 120° ) ...

Of particular interest is the

**ratio**of maximum shadow elevation to observer ' selevation 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 or ~ 120° ) ...

Page 222

75 0 - 0 - 0 . 5 critical Roche surface for mass

cm . li o ? ? _ 3 _ 10 " сm I division Fig . 6 . - The locations in the orbital plane ( as

projected for i = 90° ) of the strong pulsation events as derived from the precise ...

75 0 - 0 - 0 . 5 critical Roche surface for mass

**ratio**= 1 . 7 0 . 25 HZ Her Her X - 11cm . li o ? ? _ 3 _ 10 " сm I division Fig . 6 . - The locations in the orbital plane ( as

projected for i = 90° ) of the strong pulsation events as derived from the precise ...

Page 227

Next , we look at the predicted Doppler velocity vs . phase for a filled Roche lobe .

These results are strongly dependent on the assumed mass

essentially independent of the assumed X - ray beam shape or the visibility

function ...

Next , we look at the predicted Doppler velocity vs . phase for a filled Roche lobe .

These results are strongly dependent on the assumed mass

**ratio**, but areessentially independent of the assumed X - ray beam shape or the visibility

function ...

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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