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

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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 58

The amount of data is small , the scatter in the raw data is rather large , and there

is a wide dispersion in the

gives a

The amount of data is small , the scatter in the raw data is rather large , and there

is a wide dispersion in the

**values**for the amplitude given by different ... 5 Ib . Thisgives a

**value**of T . = 22 500° , and a linear limb - darkening coefficient of u = 0 .Page 59

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

correspond to the larger

0 .

**values**of Q . The smaller**values**of Q are acceptable only if the observed**values**of K 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 0 . 250 .

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### Contents

Gruppo fotografico del partecipanti al Corso | 1 |

Introduction | 17 |

Сen | 37 |

Copyright | |

61 other sections not shown

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### Common terms and phrases

accretion amplitude angular antenna approximation assumed Astrophys binary black hole calculations condition considered cooling core corresponding density depends detailed detectors determined dips discussed disk distance eclipse effect electron emission energy equation estimate existence expected field flux frequency function given gives gravitational heating important increase indicated intensity interesting Journ less Lett light curve limit lines luminosity magnetic field mass matter mean measured momentum motion Nature neutrino neutron star object observed obtained occur optical orbital parameters particle period phase photons Phys physical plasma possible potential present pressure problem pulsations radiation radio radius range region relation relative rotating scale sensitivity shown shows solution spectrum stellar stellar wind suggested surface temperature values variable variations velocity X-ray source