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

### From inside the book

Results 1-3 of 77

Page 54

The lower mass

larger values of Mx are now allowed . ... An upper

determined for the projected velocity Vopt sin i [ 33 ] , based on a small number of

observations ...

The lower mass

**limit**does not change by allowing smaller values of 0 . , butlarger values of Mx are now allowed . ... An upper

**limit**of 50 km / s wasdetermined for the projected velocity Vopt sin i [ 33 ] , based on a small number of

observations ...

Page 95

Cygnus X - 3 has not yet been detected at visual or near - infra - red ( 2 < l um )

wavelengths , but some useful

simple models . A

Hale ...

Cygnus X - 3 has not yet been detected at visual or near - infra - red ( 2 < l um )

wavelengths , but some useful

**limits**have been set that can be compared withsimple models . A

**limit**of about V > 21 mag was set by a group [ 188 ] using theHale ...

Page 627

1 ) P , ( cos 6 ) , and su = m ( ia ) , Vai = m ( 1 + 1 ) ( ia / 2 ) , 231 = } m ( 212 + 41 +

3 ) ( ia / 3 ) , where g = r sin 0 , 2 = r cos 0 . The 1 = 2 moments are found to ...

**limit**, Es can be expanded in spherical harmonies as [ 9 ] ( 2 . 3 ) 5o = Eboir + 1 +1 ) P , ( cos 6 ) , and su = m ( ia ) , Vai = m ( 1 + 1 ) ( ia / 2 ) , 231 = } m ( 212 + 41 +

3 ) ( ia / 3 ) , where g = r sin 0 , 2 = r cos 0 . The 1 = 2 moments are found to ...

### What people are saying - Write a review

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

### Contents

Gruppo fotografico del partecipanti al Corso | 1 |

Introduction | 17 |

Сen | 37 |

Copyright | |

61 other sections not shown

### Other editions - View all

### 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