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Mechanism for X-ray production in extars

Published online by Cambridge University Press:  14 August 2015

O. P. Manley  and
S. Olbert
O. P. Manley
Affiliation:
American Science and Engineering
S. Olbert
Affiliation:
Massachusetts Institute of Technology

Extract

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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

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