Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 270
Figure 7 shows intensity variations in Cygnus X - 2 with a change of about 50 %
in about 0 . 3 days and statistically significant fluctuations throughout . Figure 8
shows observations of GX17 + 2 on 2 different days . The first day ' s data ...
Figure 7 shows intensity variations in Cygnus X - 2 with a change of about 50 %
in about 0 . 3 days and statistically significant fluctuations throughout . Figure 8
shows observations of GX17 + 2 on 2 different days . The first day ' s data ...
Page 278
from the Vela satellites determine the turn - on to better than a day with a rise of
over a factor of 100 in intensity . The spectral and intensity variations used to rule
out a simple expanding shell can be seen in the data . Figure 15 shows 2 years ...
from the Vela satellites determine the turn - on to better than a day with a rise of
over a factor of 100 in intensity . The spectral and intensity variations used to rule
out a simple expanding shell can be seen in the data . Figure 15 shows 2 years ...
Page 318
The computations of the emitted gravitational radiation are given on the right -
hand side of the figure . The solid lines indicate the results of the simultaneous
integration of eqs . ( 1 ) and ( 2 ) . The dashed lines on the left - hand side do not
...
The computations of the emitted gravitational radiation are given on the right -
hand side of the figure . The solid lines indicate the results of the simultaneous
integration of eqs . ( 1 ) and ( 2 ) . The dashed lines on the left - hand side do not
...
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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 |