Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 67
The extensive investigations of Mc CRAY and his co - workers have shown that
the study of ultraviolet emission lines should also be very informative . We note ,
for convenience in comparing with X - ray measurements which are usually ...
The extensive investigations of Mc CRAY and his co - workers have shown that
the study of ultraviolet emission lines should also be very informative . We note ,
for convenience in comparing with X - ray measurements which are usually ...
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 ratio of ...
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 ratio of ...
Page 103
Measurements of the phase dependence of the linear polarization in the Herculis
system would be of interest . 124 . Satellite UV observations . – Satellite studies
of the shape of the ultraviolet continuum from Sco X - 1 can be used to help ...
Measurements of the phase dependence of the linear polarization in the Herculis
system would be of interest . 124 . Satellite UV observations . – Satellite studies
of the shape of the ultraviolet continuum from Sco X - 1 can be used to help ...
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Contents
Gruppo fotografico del partecipanti al Corso | 1 |
Introduction | 17 |
Сen | 37 |
Copyright | |
59 other sections not shown
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absorption accretion amplitude analysis angular approximation assumed Astrophys binary black hole calculations charge considered convective core corresponding cycle density dependence detailed detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate evolution existence expected field Figure flux frequency function geometry give given gravitational important increase indicated intensity interesting Journ less Lett light curve limit lines magnetic mass mean measurements motion Nature neutrino neutron star observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations radiation radio range ratio region relation relative rotating scale sensitivity shell shown shows solutions spectrum stellar stellar wind structure suggested surface temperature values variable variations velocity X-ray sources