Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 92
The optical spectrum of V 818 Sco does not show strong sharp stellar absorption
lines like those present in the other identified binary X - ray sources . Instead , the
spectrum exhibits ( 155 , 156 , 161 - 164 ) a very blue continuum with weak ...
The optical spectrum of V 818 Sco does not show strong sharp stellar absorption
lines like those present in the other identified binary X - ray sources . Instead , the
spectrum exhibits ( 155 , 156 , 161 - 164 ) a very blue continuum with weak ...
Page 93
The radial velocities inferred from Hell 24686 give weak evidence [ 171 ] that the
phase of closest approach of the region emitting this line may agree with the
phase of maximum light . 8o5 . Distance . - The distance to Sco X - 1 is uncertain .
The radial velocities inferred from Hell 24686 give weak evidence [ 171 ] that the
phase of closest approach of the region emitting this line may agree with the
phase of maximum light . 8o5 . Distance . - The distance to Sco X - 1 is uncertain .
Page 294
and magnetic lines of force introducing at every point the line tangent to the
direction of the electric and of the magnetic field . It is possible to show that these
lines coincide with the lines of constant flux [ 43 ] defined by the equations F u dv
...
and magnetic lines of force introducing at every point the line tangent to the
direction of the electric and of the magnetic field . It is possible to show that these
lines coincide with the lines of constant flux [ 43 ] defined by the equations F u dv
...
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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 |