Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 72
The variable emission line Hell 24686 was discovered by BOLTON ( 15 ) , and it
has been suggested [ 22 , 23 , 27 ] that the velocities of this emission line are in
antiphase with the stellar absorption line velocities . SMITH , MORGAN and ...
The variable emission line Hell 24686 was discovered by BOLTON ( 15 ) , and it
has been suggested [ 22 , 23 , 27 ] that the velocities of this emission line are in
antiphase with the stellar absorption line velocities . SMITH , MORGAN and ...
Page 98
The equivalent width of the interstellar Ca II K - line suggests a distance of about
2 . ... 205 , 211 ] have suggested other values within this range , although one
group [ 218 ] has proposed a value as high as 40 M , on the basis of an assumed
...
The equivalent width of the interstellar Ca II K - line suggests a distance of about
2 . ... 205 , 211 ] have suggested other values within this range , although one
group [ 218 ] has proposed a value as high as 40 M , on the basis of an assumed
...
Page 114
0 ) suggested a system with three luminosity sources : the relatively cool
backside of the primary star , its heated face which is ... In the present discussion
we suggest that various bumps , shoulders , peaks , the shape of primary minima
and ...
0 ) suggested a system with three luminosity sources : the relatively cool
backside of the primary star , its heated face which is ... In the present discussion
we suggest that various bumps , shoulders , peaks , the shape of primary minima
and ...
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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 |