Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page xxii
The launch of the first orbiting X-ray telescope by B. Giacconi and his group in
1971 opened a new trend in the study of the physics and astrophysics of neutron
stars and black holes. The discovery of many binary X-ray sources from by the ...
The launch of the first orbiting X-ray telescope by B. Giacconi and his group in
1971 opened a new trend in the study of the physics and astrophysics of neutron
stars and black holes. The discovery of many binary X-ray sources from by the ...
Page 18
I believe that this will be necessary if we are indeed to use binary X-ray stars as
astrophysical laboratories to study ... Such accretion disks are also normally
invoked to explain X-ray emission from binary sources containing a black hole.
I believe that this will be necessary if we are indeed to use binary X-ray stars as
astrophysical laboratories to study ... Such accretion disks are also normally
invoked to explain X-ray emission from binary sources containing a black hole.
Page 288
Once again the fundamental step was achieved with direct experimental
observations : the discovery of binary X - ray sources from the Uhuru satellite in
1971 [ 5 , 11 ] . The observations by GIACCONI and his co - workers clearly
demonstrated ...
Once again the fundamental step was achieved with direct experimental
observations : the discovery of binary X - ray sources from the Uhuru satellite in
1971 [ 5 , 11 ] . The observations by GIACCONI and his co - workers clearly
demonstrated ...
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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 |