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

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Page 48

The

types of

surface , the second related to the local stellar atmospheres . The simplest ...

The

**approximation**breaks down when R / R . ~ 1 . Due to the azimuthal ... Twotypes of

**approximations**are commonly made , the first related to the shape of thesurface , the second related to the local stellar atmospheres . The simplest ...

Page 49

Furthermore , this

explained below , is entirely inadequate in discussions of X - ray heating effects .

A somewhat more sophisticated geometrical

Furthermore , this

**approximation**always yields two equal light minima , and , asexplained below , is entirely inadequate in discussions of X - ray heating effects .

A somewhat more sophisticated geometrical

**approximation**is the expansion in ...Page 495

The method employed can be called mean - field

alternatively , a relativistic Hartree

pure vector interaction by ZELDOVICH [ 43 ] , who made an extensive study of

the high ...

The method employed can be called mean - field

**approximation**, or ,alternatively , a relativistic Hartree

**approximation**[ 42 ] . It was first employed for apure vector interaction by ZELDOVICH [ 43 ] , who made an extensive study of

the high ...

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### Contents

Why are the stars as they are? | 1 |

Krzeminskis StarCen | 5 |

The theory of degenerate configurations the limiting | 7 |

Copyright | |

64 other sections not shown

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### Common terms and phrases

absorption accretion amplitude analysis antenna approximation assumed Astrophys BAHCALL binary black hole calculated colors considered consistent core corresponding cycle Cyg X-1 density dependence detail detected detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate existence expected field Figure flux frequency function geometry give given gravitational gravitational collapse important increases indicated intensity interesting Journ less Lett light curve limit lines magnetic mass measurements motion Nature neutron star noise observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations pulse radiation radio range ratio region relative rotation scale sensitivity shown shows spectrum stellar stellar wind suggested surface temperature transducer values variable variations velocity X-ray sources