Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 18
Shorter time scales (10~3s) give us information about events occurring very close
to the surface of the star (10' cm), ... In the case of stellar-wind accretion, as is
believed to occur in Cen X-3, shocks and accretion wakes dominate a region of ...
Shorter time scales (10~3s) give us information about events occurring very close
to the surface of the star (10' cm), ... In the case of stellar-wind accretion, as is
believed to occur in Cen X-3, shocks and accretion wakes dominate a region of ...
Page 251
In the case of the Vela satellites a trigger occurs , and therefore data exist , only if
the flux rises rapidly at some point . Clearly , if the ... We can , therefore , give only
an upper limit to the time in which significant changes occur in the energy flux .
In the case of the Vela satellites a trigger occurs , and therefore data exist , only if
the flux rises rapidly at some point . Clearly , if the ... We can , therefore , give only
an upper limit to the time in which significant changes occur in the energy flux .
Page 400
Beyond this point a thermal runaway presumably occurs . ... This value
approaches that required for a beta - induced reimplosion and leaves open the
possibility that for low enough initial 12C abundance remnant formation may
occur .
Beyond this point a thermal runaway presumably occurs . ... This value
approaches that required for a beta - induced reimplosion and leaves open the
possibility that for low enough initial 12C abundance remnant formation may
occur .
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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 |