Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 376
After the fuel in a convective core is exhausted , neutrino cooling causes
gravitational contraction . If the mass of the convective core is larger than the
ignition mass for the burning of the ashes of the fuel just consumed , the next
burning stage ...
After the fuel in a convective core is exhausted , neutrino cooling causes
gravitational contraction . If the mass of the convective core is larger than the
ignition mass for the burning of the ashes of the fuel just consumed , the next
burning stage ...
Page 395
1 ' 8 , 1 ' 9 we have shown that , for at least one simple model of convection in a
Urca region , it is possible to construct a self ... In the foregoing analysis the
assumption of a steady state for the convective core was of vital importance .
1 ' 8 , 1 ' 9 we have shown that , for at least one simple model of convection in a
Urca region , it is possible to construct a self ... In the foregoing analysis the
assumption of a steady state for the convective core was of vital importance .
Page 412
He shell : X ( Q ) , convective 0 . 804 convective 0 . 720 0 . 235 5 . 83 ( 2 ) 3 . 64 (
33 ) 3 . 40 ( 9 ) convective 0 . 936 0 . 199 2 . 89 ( 2 ) 9 . 78 ( 33 ) 8 . 71 ( 9 )
convective 0 . 928 0 . 270 4 . 76 ( 2 ) 2 . 43 ( 34 ) 1 . 07 ( 10 ) 0 . 392 1 . 05 ( 3 ) 4 .
He shell : X ( Q ) , convective 0 . 804 convective 0 . 720 0 . 235 5 . 83 ( 2 ) 3 . 64 (
33 ) 3 . 40 ( 9 ) convective 0 . 936 0 . 199 2 . 89 ( 2 ) 9 . 78 ( 33 ) 8 . 71 ( 9 )
convective 0 . 928 0 . 270 4 . 76 ( 2 ) 2 . 43 ( 34 ) 1 . 07 ( 10 ) 0 . 392 1 . 05 ( 3 ) 4 .
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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 |