Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 48
The approximation breaks down when R / R . ~ 1 . Due to the azimuthal ... Two
types of approximations are commonly made , the first related to the shape of the
surface , the second related to the local stellar atmospheres . The simplest ...
The approximation breaks down when R / R . ~ 1 . Due to the azimuthal ... Two
types of approximations are commonly made , the first related to the shape of the
surface , the second related to the local stellar atmospheres . The simplest ...
Page 49
Furthermore , this approximation always yields two equal light minima , and , as
explained below , is entirely inadequate in discussions of X - ray heating effects .
A somewhat more sophisticated geometrical approximation is the expansion in ...
Furthermore , this approximation always yields two equal light minima , and , as
explained 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 approximation , or ,
alternatively , a relativistic Hartree approximation [ 42 ] . It was first employed for a
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 a
pure 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
Bibliographic information
| Title | Proceedings of the International School of Physics "Enrico Fermi.", Volume 65 Proceedings of the International School of Physics "Enrico Fermi.", Società italiana di fisica Rivista del nuovo cimento |
| Contributor | Società italiana di fisica |
| Publisher | N. Zanichelli, 1978 |
| Original from | the University of California |
| Digitized | 14 Aug 2008 |
| ISBN | 0720407206, 9780720407204 |
| Export Citation | BiBTeX EndNote RefMan |