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

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Page 170

10 - 21 cm2 Hz . With given values of cross - section and noise

( 1 ) gives the minimum energy spectral density of pulses which could be

detected . Assuming that the antenna

noise ...

10 - 21 cm2 Hz . With given values of cross - section and noise

**temperature**, eq .( 1 ) gives the minimum energy spectral density of pulses which could be

detected . Assuming that the antenna

**temperature**were low enough for resonatornoise ...

Page 418

The numerical results are similar if we take the sound traversal time for the

convective region explicitly from numerical models . The characteristic time for

E , is ...

The numerical results are similar if we take the sound traversal time for the

convective region explicitly from numerical models . The characteristic time for

**temperature**increase due to the nuclear reactions is ( 24 ) Tin Tym = E - T , whereE , is ...

Page 808

An alternative self - consistent solution exists , however , in which the ion and

electron

two -

ions ...

An alternative self - consistent solution exists , however , in which the ion and

electron

**temperatures**are not equal , but ... The main assumption underlying thetwo -

**temperature**disk structure ( in addition to those discussed above ) is thations ...

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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