Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 156
One of these is the precise measurement of their positions in the clusters . Every
hypothesis ... Precise position measurements on 5 sources should therefore yield
a mean radial distance related to the mean mass of the sources . The MIT group ...
One of these is the precise measurement of their positions in the clusters . Every
hypothesis ... Precise position measurements on 5 sources should therefore yield
a mean radial distance related to the mean mass of the sources . The MIT group ...
Page 159
Variability and position of the compact X - ray sources in Cen A . Centaurus A (
NGC 5128 ) , the nearest radio galaxy , has an active nucleus which appears to
have ejected two collinear pairs of radio lobes , an outer pair spanning 5° and an
...
Variability and position of the compact X - ray sources in Cen A . Centaurus A (
NGC 5128 ) , the nearest radio galaxy , has an active nucleus which appears to
have ejected two collinear pairs of radio lobes , an outer pair spanning 5° and an
...
Page 253
Two positions are equally likely for the source of each GRB . One of those for 72 -
2 has a most probable position within a degree of that of Cygnus X - 1 , the
probable error being two or three degrees . Although there is no other known X -
ray ...
Two positions are equally likely for the source of each GRB . One of those for 72 -
2 has a most probable position within a degree of that of Cygnus X - 1 , the
probable error being two or three degrees . Although there is no other known X -
ray ...
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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 |