Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 238
In this model , the neutron star moves supersonically through a stellar wind , and
accretes material from it via a dense accretion wake which forms by gravitational
focussing behind the neutron star ( fig . 7 ) . a Fig . 7 . - Schematic representation
...
In this model , the neutron star moves supersonically through a stellar wind , and
accretes material from it via a dense accretion wake which forms by gravitational
focussing behind the neutron star ( fig . 7 ) . a Fig . 7 . - Schematic representation
...
Page 743
Accretion of the stellar wind . 61 . Capture of the stellar wind . - A stellar wind with
velocity V . and density N , is assumed to exist , which is flowing around a
relativistic star of mass Mx : The radius of gravitational capture is assumed to be
equal ...
Accretion of the stellar wind . 61 . Capture of the stellar wind . - A stellar wind with
velocity V . and density N , is assumed to exist , which is flowing around a
relativistic star of mass Mx : The radius of gravitational capture is assumed to be
equal ...
Page 753
Nonstationary accretion of stellar wind . It was mentioned in subsect . 6 * 2 that ,
for low velocities of the stellar wind , the effects of accreting - plasma heating by X
- ray radiation makes impossible the picture of stationary accretion . Possible ...
Nonstationary accretion of stellar wind . It was mentioned in subsect . 6 * 2 that ,
for low velocities of the stellar wind , the effects of accreting - plasma heating by X
- ray radiation makes impossible the picture of stationary accretion . Possible ...
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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 |