Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 182
In this way it would be possible to reach about 3 mK at the cost of greater
complexity and by sacrificing continuous operation . It appears that , with present
techniques , the overall Q may be limited by flux motion losses in
superconducting ...
In this way it would be possible to reach about 3 mK at the cost of greater
complexity and by sacrificing continuous operation . It appears that , with present
techniques , the overall Q may be limited by flux motion losses in
superconducting ...
Page 641
In previous reviews [ 3 , 7 ] , it was concluded that older pulsars are as cold as ~ (
103 - 105 ) K . The various possible heating effects were not taken into account ,
mostly because realistic estimates seemed almost impossible . It is possible that
...
In previous reviews [ 3 , 7 ] , it was concluded that older pulsars are as cold as ~ (
103 - 105 ) K . The various possible heating effects were not taken into account ,
mostly because realistic estimates seemed almost impossible . It is possible that
...
Page 753
Possible nonstationary accretion regimes are considered below . It should be
mentioned that these regimes are possible in binaries with low velocities of the
stellar wind . Since the stellar - wind velocity is usually close , in order of
magnitude ...
Possible nonstationary accretion regimes are considered below . It should be
mentioned that these regimes are possible in binaries with low velocities of the
stellar wind . Since the stellar - wind velocity is usually close , in order of
magnitude ...
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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 |