Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 69
8 h for Cyg X - 3 ) that is interpreted as orbital motion in a binary system of stars .
This motion determines the so - called mass function ( according to the following
straightforward result of Newton ' s laws for elliptical orbits ) m sinį ( r , sin i ) ...
8 h for Cyg X - 3 ) that is interpreted as orbital motion in a binary system of stars .
This motion determines the so - called mass function ( according to the following
straightforward result of Newton ' s laws for elliptical orbits ) m sinį ( r , sin i ) ...
Page 115
3 that the orbits corresponding to the two symmetry points are themselves
symmetric in orbital phase . Thus there are actually 4 symmetry points ,
corresponding to q = 0 . 0 and q = 0 . 5 in each of the two symmetric light curves .
) Since we are ...
3 that the orbits corresponding to the two symmetry points are themselves
symmetric in orbital phase . Thus there are actually 4 symmetry points ,
corresponding to q = 0 . 0 and q = 0 . 5 in each of the two symmetric light curves .
) Since we are ...
Page 138
Figure 17 clearly implies that to produce a 7 orbit ( 12 day or ~ 120° ) period in
which X - rays are observed implies an elevation ... The large departure of the
disk from the orbital plane implied by the optical data is strongly dependent on
the ...
Figure 17 clearly implies that to produce a 7 orbit ( 12 day or ~ 120° ) period in
which X - rays are observed implies an elevation ... The large departure of the
disk from the orbital plane implied by the optical data is strongly dependent on
the ...
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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 |