Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 487
... in the following way : the authors define an even - and an odd - state potential
such that the even one is the same as the D2 - potential for the NN case and the
odd one is a spin - isospin average of the 3P , - state NN potential ( less OPEP ) .
... in the following way : the authors define an even - and an odd - state potential
such that the even one is the same as the D2 - potential for the NN case and the
odd one is a spin - isospin average of the 3P , - state NN potential ( less OPEP ) .
Page 835
Algol type this is not the case : the main - sequence component is always the
more massive one , whereas the ( more evolved ) subgiant is the less massive
one . For instance , in the case of Algol , the main - sequence component ( B8 )
has a ...
Algol type this is not the case : the main - sequence component is always the
more massive one , whereas the ( more evolved ) subgiant is the less massive
one . For instance , in the case of Algol , the main - sequence component ( B8 )
has a ...
Page 837
( As long as the mass less is not violent , and we are not dealing with contact
systems — in which the rotational and orbital angular momenta are of
comparable order of magnitude , these assumptions seem reasonably well
justified . ) c ) The ...
( As long as the mass less is not violent , and we are not dealing with contact
systems — in which the rotational and orbital angular momenta are of
comparable order of magnitude , these assumptions seem reasonably well
justified . ) c ) The ...
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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 |