Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 517
We shall , therefore , view a pulsar as a rapidly rotating magnetized sphere with
the axis of rotation 2 inclined by an angle « with respect to the magneticfield axis
( fig . 1 ) . If we now believe that the fast rotating pulsar at the center of the Crab ...
We shall , therefore , view a pulsar as a rapidly rotating magnetized sphere with
the axis of rotation 2 inclined by an angle « with respect to the magneticfield axis
( fig . 1 ) . If we now believe that the fast rotating pulsar at the center of the Crab ...
Page 644
A Numerical Study of Rotating Relativistic Stars ( “ ) . J . R . WILSON Lawrence
Livermore Laboratory , University of California - Livermore , Cal . 94550 1 . –
Introduction . Rotating supermassive stars have been long considered as
possible ...
A Numerical Study of Rotating Relativistic Stars ( “ ) . J . R . WILSON Lawrence
Livermore Laboratory , University of California - Livermore , Cal . 94550 1 . –
Introduction . Rotating supermassive stars have been long considered as
possible ...
Page 659
profile is uniformly stretched by a small amount in the R - direction and the whole
iteration process is repeated until an equilibrium is achieved . This develops a
sequence of faster and faster rotating stars with about the same central densities .
profile is uniformly stretched by a small amount in the R - direction and the whole
iteration process is repeated until an equilibrium is achieved . This develops a
sequence of faster and faster rotating stars with about the same central densities .
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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.", Societą italiana di fisica Rivista del nuovo cimento |
| Contributor | Societą 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 |