Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 97
... within a single night [ 199 ] and data from different lines yield significantly
divergent velocities [ 206 ] . The values of the K - velocity in the literature range [
204 , 206 ] from 37 km / s to 23 km / s and the quoted eccentricities range from 0
to 0 .
... within a single night [ 199 ] and data from different lines yield significantly
divergent velocities [ 206 ] . The values of the K - velocity in the literature range [
204 , 206 ] from 37 km / s to 23 km / s and the quoted eccentricities range from 0
to 0 .
Page 157
Light curves of the 104 s pulsations of the transient X - ray source A0535 + 26 in
two energy ranges as measured by SAS ... modulation at all energies is about 30
% , but the detailed features change markedly over the observed energy range ...
Light curves of the 104 s pulsations of the transient X - ray source A0535 + 26 in
two energy ranges as measured by SAS ... modulation at all energies is about 30
% , but the detailed features change markedly over the observed energy range ...
Page 163
Behind each collimator a bank of proportional counters sensitive to X - rays in the
energy range from 2 to 10 keV is mounted . When the observatory rotates about
its z - axis , the flux of X - rays reaching the counters from a given X - ray source ...
Behind each collimator a bank of proportional counters sensitive to X - rays in the
energy range from 2 to 10 keV is mounted . When the observatory rotates about
its z - axis , the flux of X - rays reaching the counters from a given X - ray source ...
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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 |