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OH Masers in Outflow Regions
Published online by Cambridge University Press: 07 August 2017
Abstract
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We combine a sophisticated model of maser propagation with a simple model of an accelerating molecular outflow and show that the observation of different OH maser frequencies is consistent with emission from different parts of the outflow.
- Type
- Quiescent Clouds and Regions of Star Formation
- Information
- Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 277 - 280
- Copyright
- Copyright © Kluwer 1992
References
REFERENCES
Baudry, A., Diamond, P., Booth, R., Graham, D. and Walmsley, C. M.
1988. Astron. & Astrophys., 201, 105.Google Scholar
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