Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 67
We note , for convenience in comparing with X - ray measurements which are usually quoted as fluxes in CGS units , that , for a V = 0.0 star , the flux F = 3.64.10-9 erg cm - ' s - 1 A - and F , = 3.65.10-20 erg cm - 25-1 Hz - 1 ( see ...
We note , for convenience in comparing with X - ray measurements which are usually quoted as fluxes in CGS units , that , for a V = 0.0 star , the flux F = 3.64.10-9 erg cm - ' s - 1 A - and F , = 3.65.10-20 erg cm - 25-1 Hz - 1 ( see ...
Page 68
Polarization measurements . Polarization measurements have not yet been extensively used in the study of binary X - ray sources , although several important studies have been carried out . In a few cases , it has been shown that the ...
Polarization measurements . Polarization measurements have not yet been extensively used in the study of binary X - ray sources , although several important studies have been carried out . In a few cases , it has been shown that the ...
Page 103
Measurements of the phase dependence of the linear polarization in the Herculis system would be of interest . 12'4 . Satellite UV observations . · Satellite studies of the shape of the ultraviolet continuum from Sco X - 1 can be used to ...
Measurements of the phase dependence of the linear polarization in the Herculis system would be of interest . 12'4 . Satellite UV observations . · Satellite studies of the shape of the ultraviolet continuum from Sco X - 1 can be used to ...
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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