Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 135
But it must be both large and tilted not only to reproduce the secondary minimum
through occultation , but also to provide the appropriate luminosity contribution
around primary minimum . The inclination of the orbit introduces a fundamental ...
But it must be both large and tilted not only to reproduce the secondary minimum
through occultation , but also to provide the appropriate luminosity contribution
around primary minimum . The inclination of the orbit introduces a fundamental ...
Page 593
1 ) and by assuming a small core ( mo , ro ) to exist above the point C up to C * ,
the mass contributions along the paths a ... It is the path c ) that gives the bigger
contribution at the very beginning ( dashed line ) , as it should according to the ...
1 ) and by assuming a small core ( mo , ro ) to exist above the point C up to C * ,
the mass contributions along the paths a ... It is the path c ) that gives the bigger
contribution at the very beginning ( dashed line ) , as it should according to the ...
Page 717
The inclination of the orbit of this system is close to 90° , therefore the contribution
of the disc radiation to the total light is small in comparison with the « hot spot »
brightness . Thus the disc emission is visible only at phases in the binary period ...
The inclination of the orbit of this system is close to 90° , therefore the contribution
of the disc radiation to the total light is small in comparison with the « hot spot »
brightness . Thus the disc emission is visible only at phases in the binary period ...
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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 |