Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 117
In an attempt to understand the time - dependent properties of the structure on
the light curve suggested in fig . 3 we have examined the power spectrum of the
1973 B data which span 255 days . Observations were binned in 40 min intervals
...
In an attempt to understand the time - dependent properties of the structure on
the light curve suggested in fig . 3 we have examined the power spectrum of the
1973 B data which span 255 days . Observations were binned in 40 min intervals
...
Page 871
73 , Structure and Evolution of Close Binary Systems ( in press ) . [ 77 ] B .
PACZYNSKI : 1976 , Proceedings of the 1 . A . U . Symposium No . 73 , Structure
and Evolution of Close Binary Systems ( in press ) . [ 78 ] M . E . ALEXANDER :
1973 ...
73 , Structure and Evolution of Close Binary Systems ( in press ) . [ 77 ] B .
PACZYNSKI : 1976 , Proceedings of the 1 . A . U . Symposium No . 73 , Structure
and Evolution of Close Binary Systems ( in press ) . [ 78 ] M . E . ALEXANDER :
1973 ...
Page
Ericson Course XXXIX Plasma Astrophysics edited by P. A. Sturrock Course XL
Nuclear Structure and Nuclear Reactions edited by M. Jean Course XLI Selected
Topics in Particle Physics edited by J. Steinberoer Course XLII Quantum Optics ...
Ericson Course XXXIX Plasma Astrophysics edited by P. A. Sturrock Course XL
Nuclear Structure and Nuclear Reactions edited by M. Jean Course XLI Selected
Topics in Particle Physics edited by J. Steinberoer Course XLII Quantum Optics ...
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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