Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 169
It is assumed that the motion is detected by a linear transducer of noise
temperature Ty . Equation ( 1 ) takes account of the three most important sources
of noise in a detector : the thermal fluctuations in the antenna , the inaccuracy
involved in ...
It is assumed that the motion is detected by a linear transducer of noise
temperature Ty . Equation ( 1 ) takes account of the three most important sources
of noise in a detector : the thermal fluctuations in the antenna , the inaccuracy
involved in ...
Page 300
The motion of a test particle of mass u and charge ε in a background
electromagnetic and gravitational field with metric guy and electromagnetic
potential A , is described by a Lagrangian [ 89 ] ( 21 ) L = 9uv ih zu – , Aais , и
where the dots ...
The motion of a test particle of mass u and charge ε in a background
electromagnetic and gravitational field with metric guy and electromagnetic
potential A , is described by a Lagrangian [ 89 ] ( 21 ) L = 9uv ih zu – , Aais , и
where the dots ...
Page 301
We can then conclude that , if S = 0 and the motion crosses the equatorial plane ,
then the motion has to be confined to the equatorial plane ; if 8 > 0 , the motion is
limited to a maximum angle out of the equatorial plane depending on the ...
We can then conclude that , if S = 0 and the motion crosses the equatorial plane ,
then the motion has to be confined to the equatorial plane ; if 8 > 0 , the motion is
limited to a maximum angle out of the equatorial plane depending on the ...
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Contents
Why are the stars as they are? | 1 |
Krzeminskis StarCen | 5 |
The theory of degenerate configurations the limiting | 7 |
Copyright | |
64 other sections not shown
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Common terms and phrases
absorption accretion amplitude analysis antenna approximation assumed Astrophys BAHCALL binary black hole calculated colors considered consistent core corresponding cycle Cyg X-1 density dependence detail detected detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate existence expected field Figure flux frequency function geometry give given gravitational gravitational collapse important increases indicated intensity interesting Journ less Lett light curve limit lines magnetic mass measurements motion Nature neutron star noise observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations pulse radiation radio range ratio region relative rotation scale sensitivity shown shows spectrum stellar stellar wind suggested surface temperature transducer 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 |