Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 18
The on-off cycles have characteristic times of the order of days or weeks, and
absorption features may last hours. 3) At still greater distances from the X-ray
source, the flow of gas from the companion star, as well as the density
dependence on ...
The on-off cycles have characteristic times of the order of days or weeks, and
absorption features may last hours. 3) At still greater distances from the X-ray
source, the flow of gas from the companion star, as well as the density
dependence on ...
Page 38
These are the absorption dips and absorption trough . The existence of
absorption dips in the light curve of Cyg X - 1 has received considerable attention
since their discovery by MASON , HAWKINS , SANFORD , MURDIN and
SAVAGE [ 38 ] ...
These are the absorption dips and absorption trough . The existence of
absorption dips in the light curve of Cyg X - 1 has received considerable attention
since their discovery by MASON , HAWKINS , SANFORD , MURDIN and
SAVAGE [ 38 ] ...
Page 67
One also would like to know the total visual absorption in order to be able to
estimate the distance to the source using the observed visual flux and luminosity
class . Reasonable distance estimates to individual sources can be obtained by ...
One also would like to know the total visual absorption in order to be able to
estimate the distance to the source using the observed visual flux and luminosity
class . Reasonable distance estimates to individual sources can be obtained by ...
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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.", 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 |