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Circular Polarization of Astrophysical Masers
Published online by Cambridge University Press: 03 August 2017
Abstract
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Results of further calculations are presented to explore the non-linear, Zeeman overlap effect as the cause for the circular polarization of astrophysical masers. Emphasis is placed on the regime in which the Zeeman splitting is small and on the variation of the polarization with maser saturation.
- Type
- Galactic
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- Copyright
- Copyright © Reidel 1988
References
Cohen, R. J., Downs, G., Emerson, R., Grimm, M., Gulkis, S., Stevens, G., and Tarter, J.
1987, MNRAS, 225, 491.Google Scholar
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