Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 156
One of these is the precise measurement of their positions in the clusters . ... Precise position measurements on 5 sources should therefore yield a mean radial distance related to the mean mass of the sources .
One of these is the precise measurement of their positions in the clusters . ... Precise position measurements on 5 sources should therefore yield a mean radial distance related to the mean mass of the sources .
Page 159
Variability and position of the compact X - ray sources in Cen A. Centaurus A ( NGC 5128 ) , the nearest radio galaxy , has an active nucleus which appears to have ejected two collinear pairs of radio lobes , an outer pair spanning 5 ...
Variability and position of the compact X - ray sources in Cen A. Centaurus A ( NGC 5128 ) , the nearest radio galaxy , has an active nucleus which appears to have ejected two collinear pairs of radio lobes , an outer pair spanning 5 ...
Page 253
Two positions are equally likely for the source of each GRB . One of those for 72-2 has a most probable position within a degree of that of Cygnus X - 1 , the probable error being two or three degrees . Although there is no other known ...
Two positions are equally likely for the source of each GRB . One of those for 72-2 has a most probable position within a degree of that of Cygnus X - 1 , the probable error being two or three degrees . Although there is no other known ...
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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 | |
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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