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OH Masers in Outflow Regions

Published online by Cambridge University Press:  07 August 2017

M. D. Gray ,
D. Field  and
R. C. Doel
M. D. Gray
Affiliation:
School of Chemistry University of Bristol Cantock's Close Bristol BS8 1TS U.K.
D. Field
Affiliation:
School of Chemistry University of Bristol Cantock's Close Bristol BS8 1TS U.K.
R. C. Doel
Affiliation:
School of Chemistry University of Bristol Cantock's Close Bristol BS8 1TS U.K.

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
Castor, J. I. 1970. Mon. Not. Roy. Astron. Soc., 149, 111.CrossRefGoogle Scholar
Doel, R. C., Gray, M. D. and Field, D. 1990. Mon. Not. Roy. Astron. Soc., 244, 504.Google Scholar
Field, D. and Gray, M. D. 1988. Mon. Not. Roy. Astron. Soc., 234, 353.CrossRefGoogle Scholar
Fouquet, J. E. and Reid, M. J. 1982. Astronomical Journal, 87, 691.CrossRefGoogle Scholar
Gaume, R. A. and Mutel, R. L. 1987. Ap. J. Supp. 65, 193.CrossRefGoogle Scholar