Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 837
The time scale for the mass exhange is tku ; this is clear since the mass loss
disturbs the thermal equilibrium of the primary ; the time scale to reach a new
equilibrium situation is then expected to be Tu ( see subsect . 36 ) . After reaching
the ...
The time scale for the mass exhange is tku ; this is clear since the mass loss
disturbs the thermal equilibrium of the primary ; the time scale to reach a new
equilibrium situation is then expected to be Tu ( see subsect . 36 ) . After reaching
the ...
Page 838
1 ) Stage 1 , 2 ) stage 2 , 3 ) stage 3 . this stage the radii of both stars expand on a
nuclear time scale . When the primary star reaches its Roche lobe . ii ) stage 2
starts , during which it transfers , on a thermal time scale , a large fraction of its ...
1 ) Stage 1 , 2 ) stage 2 , 3 ) stage 3 . this stage the radii of both stars expand on a
nuclear time scale . When the primary star reaches its Roche lobe . ii ) stage 2
starts , during which it transfers , on a thermal time scale , a large fraction of its ...
Page 857
8 in separation ( and by a factor 14 in orbital period ) on a thermal time scale of
the primary star ( 10 * y ) implies that co - rotation cannot be maintained during
the mass exchange . On such a short time scale , tidal forces are certainly unable
to ...
8 in separation ( and by a factor 14 in orbital period ) on a thermal time scale of
the primary star ( 10 * y ) implies that co - rotation cannot be maintained during
the mass exchange . On such a short time scale , tidal forces are certainly unable
to ...
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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 |