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Mechanism for X-ray production in extars
Published online by Cambridge University Press: 14 August 2015
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This presentation attempts to describe in very qualitative terms a theory of production of high energy radiation (soft and hard X-rays) in magnetoactive plasmas of astrophysical interest. Special emphasis has been placed on the application of our model to extars and in particular to Sco X-1. More rigorous arguments may be found elsewhere [1] and the interested reader is urged to consult that reference for more details.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 413 - 423
- Copyright
- Copyright © Reidel 1970
References
[2]
Ginzburg, V. L. and Svrovatskii, S. I.: 1964, Origin of Cosmic Rays, Pergamon Press, New York.Google Scholar
[4]
Manley, O. P. and Olbert, S.: 1968, presented at Asilomar Conference on Plasma Instabilities in Astrophysics, California, October.Google Scholar
[12]
Fritz, G., Meekins, J. F., Henry, R. C., Byram, E. T., and Friedman, H.: 1968, Astrophys. J. Letters
153, L199.Google Scholar
[13]
Buselli, G., Clancy, M. C., Davison, P. J. N., Edwards, P. J., McCracken, K. G., and Thomas, R. M.: 1968, Nature
219, 5159.Google Scholar