Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 29
one 35 d cycle , by Joss et al . [ 16 ] have shown little change in the pulse shape
during the largest fraction of the « on » cycle , except during the last three days
when the fraction pulse decreased significantly . JONES et al . [ 17 ] have ...
one 35 d cycle , by Joss et al . [ 16 ] have shown little change in the pulse shape
during the largest fraction of the « on » cycle , except during the last three days
when the fraction pulse decreased significantly . JONES et al . [ 17 ] have ...
Page 115
This conclusion is supported by the obvious agreement between data from many
different 354 cycles which are superposed to ... If these features move regularly (
coherently ) from 35 ' cycle to 350 cycle this slope must be a ratio of integers ...
This conclusion is supported by the obvious agreement between data from many
different 354 cycles which are superposed to ... If these features move regularly (
coherently ) from 35 ' cycle to 350 cycle this slope must be a ratio of integers ...
Page 236
Figure 6 shows the HE and LE light curves of the well - known X - ray binary Cen
X - 3 , throughout 8 binary cycles . ... 1 ) A low and variable X - ray intensity in
cycles 2 - 4 , with a peak count rate not exceeding ( 30 - 70 ) s - 1 in any cycle .
Figure 6 shows the HE and LE light curves of the well - known X - ray binary Cen
X - 3 , throughout 8 binary cycles . ... 1 ) A low and variable X - ray intensity in
cycles 2 - 4 , with a peak count rate not exceeding ( 30 - 70 ) s - 1 in any cycle .
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Contents
Gruppo fotografico del partecipanti al Corso | 1 |
Introduction | 17 |
Сen | 37 |
Copyright | |
59 other sections not shown
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Common terms and phrases
absorption accretion amplitude analysis angular approximation assumed Astrophys binary black hole calculations charge considered convective core corresponding cycle density dependence detailed detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate evolution existence expected field Figure flux frequency function geometry give given gravitational important increase indicated intensity interesting Journ less Lett light curve limit lines magnetic mass mean measurements motion Nature neutrino neutron star observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations radiation radio range ratio region relation relative rotating scale sensitivity shell shown shows solutions spectrum stellar stellar wind structure suggested surface temperature 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.", Societą italiana di fisica Rivista del nuovo cimento |
| Contributor | Societą 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 |