Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 3
pressure due to it is given by ( 1 ) Pea Pgas =MH07 . where k denotes the
Boltzmann constant , H the mass of the hydrogen atom , u the mean molecular
weight , the density and T the temperature . The pressure due to radiation , in the
same ...
pressure due to it is given by ( 1 ) Pea Pgas =MH07 . where k denotes the
Boltzmann constant , H the mass of the hydrogen atom , u the mean molecular
weight , the density and T the temperature . The pressure due to radiation , in the
same ...
Page 18
I believe that this will be necessary if we are indeed to use binary X-ray stars as
astrophysical laboratories to study ultimately the equation of state of matter at
nuclear densities or the properties of black holes. I have assumed as a starting
point ...
I believe that this will be necessary if we are indeed to use binary X-ray stars as
astrophysical laboratories to study ultimately the equation of state of matter at
nuclear densities or the properties of black holes. I have assumed as a starting
point ...
Page 498
The energy shift increases with density and goes from + 140 to + 400 MeV , in the
density region 0 . 5 < ng < 5 ( fm - 3 ' , even in the absence of a two - body
interaction . The effect is of a general nature and is therefore expected to hold for
any ...
The energy shift increases with density and goes from + 140 to + 400 MeV , in the
density region 0 . 5 < ng < 5 ( fm - 3 ' , even in the absence of a two - body
interaction . The effect is of a general nature and is therefore expected to hold for
any ...
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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 |