Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
From inside the book
Results 1-3 of 78
Page 18
It is useful to distinguish several physically relevant regions in the discussion. 1)
For neutron stars it is important to consider the region inside the Alfven surface,
defined as the locus of points about the neutron star where the magnetic-energy
...
It is useful to distinguish several physically relevant regions in the discussion. 1)
For neutron stars it is important to consider the region inside the Alfven surface,
defined as the locus of points about the neutron star where the magnetic-energy
...
Page 386
the ( 0 - T ) - plane has been divided into five regions , the boundaries of which
are dependent at least to some extent on the ... In regions A , C and D it is mainly
the electron captures which determine the rate of neutronization , in region B ...
the ( 0 - T ) - plane has been divided into five regions , the boundaries of which
are dependent at least to some extent on the ... In regions A , C and D it is mainly
the electron captures which determine the rate of neutronization , in region B ...
Page 810
two - temperature region , cool - disk region Thole Po > P III 1 < / 8 < 3 6 . Dr . > 1
1 . < 1 1 > 1 . > 1 3300 28 b ) Des . > X . xes > * xs > < . xes < * 48 Fig . 3 . - a ) A
side view ( to scale ) of the inner portions of an accretion disk around a ...
two - temperature region , cool - disk region Thole Po > P III 1 < / 8 < 3 6 . Dr . > 1
1 . < 1 1 > 1 . > 1 3300 28 b ) Des . > X . xes > * xs > < . xes < * 48 Fig . 3 . - a ) A
side view ( to scale ) of the inner portions of an accretion disk around a ...
What people are saying - Write a review
We haven't found any reviews in the usual places.
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
Other editions - View all
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 |