Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
From inside the book
Results 1-3 of 62
Page 153
Last summer , MARKERT found that a variable , hard , high - galactic - latitude
source MX0513 — 40 , discovered by ... 7 data on 3U1820 — 30 , reported in the
3U catalogue as variables and associated with the globular cluster NGC6624 .
Last summer , MARKERT found that a variable , hard , high - galactic - latitude
source MX0513 — 40 , discovered by ... 7 data on 3U1820 — 30 , reported in the
3U catalogue as variables and associated with the globular cluster NGC6624 .
Page 189
The variable central radio source has exhibited differences in flaring behavior
between the time period 1970 - 71 and 1973 - 75 . When first discovered as a
radio source [ 2 ] , the central radio source was basically continuously variable .
The variable central radio source has exhibited differences in flaring behavior
between the time period 1970 - 71 and 1973 - 75 . When first discovered as a
radio source [ 2 ] , the central radio source was basically continuously variable .
Page 531
o , and introducing in place of r the independent variable r * defined by d d ( 25 )
drt p2 t æ2 dr ' and further changing the dependent variable g to ( 26 ) 0 = 402 (
72 + 22 ) R , we find that eq . ( 19 ) becomes d ' O ( 27 ) 211 – ( r - M ) ( r2 + Q ? ) ...
o , and introducing in place of r the independent variable r * defined by d d ( 25 )
drt p2 t æ2 dr ' and further changing the dependent variable g to ( 26 ) 0 = 402 (
72 + 22 ) R , we find that eq . ( 19 ) becomes d ' O ( 27 ) 211 – ( r - M ) ( r2 + Q ? ) ...
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 |