The diffuse cosmic X-ray background spectrum in the 2–10 keV energy range
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF02637175.pdf
Reference16 articles.
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2. Baxter, A. J., Wilson, B. G., and Green, D. W.: 1969b,Can. J. Phys. 47, 2651.
3. Boldt, E. A., Desai, U. D., Holt, S. S., and Serlemitsos, P. J.: 1969.Nature 224, 677.
4. Bunner, A. N., Coleman, P. C., Krausshaar, W. L., McCammon, D., Palmieri, T. M., Shilepsky, A., and Ulmer, M.: 1969,Nature 223, 1222.
5. Cunningham, C., Groves, D., Price, R., Rodrigues, R., Swift, C., and Mark, H. 1970,Astrophys. J. 160, 1177.
Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Ariel 5 hard X-ray measurements of galactic and extragalactic X-ray sources;Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences;1976-10
2. Annihilation of matter and antimatter and the cosmic X-ray background;Nature;1976-03
3. The X and γ diffuse background;La Rivista del Nuovo Cimento;1975-04
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