Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 306
All these topics have been treated by adopting very idealized gedanken
experiments with test particles , which should not be considered in themselves of
any realistic astrophysical meaning . Some of the conclusions , however ,
reached on ...
All these topics have been treated by adopting very idealized gedanken
experiments with test particles , which should not be considered in themselves of
any realistic astrophysical meaning . Some of the conclusions , however ,
reached on ...
Page 316
... determination of the Green ' s functions for the coupled system of equations
have been given in ref . [ 135 ] . The gravitationally induced electromagnetic
radiation , for the specific example here considered , has been found to be AE ~ 0
.
... determination of the Green ' s functions for the coupled system of equations
have been given in ref . [ 135 ] . The gravitationally induced electromagnetic
radiation , for the specific example here considered , has been found to be AE ~ 0
.
Page 326
4 cannot be considered a reliable first approximation as soon as accretion rates
as high as d M / dt ~ ~ 1017 g / s are considered . In this case a more complex
magnetohydrodynamical analysis is needed . In a classical work DEUTSCH [ 158
] ...
4 cannot be considered a reliable first approximation as soon as accretion rates
as high as d M / dt ~ ~ 1017 g / s are considered . In this case a more complex
magnetohydrodynamical analysis is needed . In a classical work DEUTSCH [ 158
] ...
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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 |