Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 161
The MIT experiment on the OSO - 7 . – The OSO - 7 was primarily a solar
observatory designed to point a collection of solar UV and X - ray telescopes at
the Sun from a platform mounted on a spinning cylindrical wheel . The latter had
seven ...
The MIT experiment on the OSO - 7 . – The OSO - 7 was primarily a solar
observatory designed to point a collection of solar UV and X - ray telescopes at
the Sun from a platform mounted on a spinning cylindrical wheel . The latter had
seven ...
Page 175
Preliminary experiments using scaled - down antennas at Stanford and Rome
have already demonstrated the expected reduction in noise when the antenna is
cooled to ... In this experiment the measured effective noise temperature was 0 .
Preliminary experiments using scaled - down antennas at Stanford and Rome
have already demonstrated the expected reduction in noise when the antenna is
cooled to ... In this experiment the measured effective noise temperature was 0 .
Page 230
Observations of Compact X - Ray Sources with the Ariel V Sky Survey
Experiment . 10 K . A . POUNDS X - Ray Astronomy Group , University of
Leicester - Leicester , England 1 . - Introduction . The Ariel V satellite was
launched into a circular ...
Observations of Compact X - Ray Sources with the Ariel V Sky Survey
Experiment . 10 K . A . POUNDS X - Ray Astronomy Group , University of
Leicester - Leicester , England 1 . - Introduction . The Ariel V satellite was
launched into a circular ...
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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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Common terms and phrases
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
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 |