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

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Page 65

In sect . 2 we describe the basic observational techniques that have been

and indicate some of the important questions which could be answered by further

( or different ) applications of the same techniques . In sect . 3 we define more ...

In sect . 2 we describe the basic observational techniques that have been

**applied**and indicate some of the important questions which could be answered by further

( or different ) applications of the same techniques . In sect . 3 we define more ...

Page 121

The coefficients in table I result from

analysis with this epoch to all available B - flux ... If the harmonic analysis is

should ...

The coefficients in table I result from

**applying**the two - dimensional harmonicanalysis with this epoch to all available B - flux ... If the harmonic analysis is

**applied**to U , B and V fluxes separately , the colors of corresponding coefficientsshould ...

Page 295

The technical program of that work was later

can be summarized in complete generality . Let go be a solution of the Einstein

equations with a momentum - energy tensor 70 . We can then define a new

metric ...

The technical program of that work was later

**applied**to black - hole physics andcan be summarized in complete generality . Let go be a solution of the Einstein

equations with a momentum - energy tensor 70 . We can then define a new

metric ...

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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