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A Thermal Source with Strong 1612 MHz OH Emission

Published online by Cambridge University Press:  25 April 2016

B. J. Robinson ,
W. M. Goss  and
R. N. Manchester
B. J. Robinson
Affiliation:
Division of Radiophysics, CSIRO, Sydney
W. M. Goss
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R. N. Manchester
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

During 1968 we have found at Parkes several types of emission in the lines of the 18 cm quadruplet of the ground-state OH molecule. This note describes a strong source of 1612 MHz emission near galactic longitude 331°.

OH emission was originally detected in the vicinity of HII regions, and a search of a large number of HII regions showed that about a third had associated OH emission. This type of emission is usually strongest at 1665 MHz, and is also seen at 1667 MHz and weakly on one of the satellite lines.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 5 , March 1969 , pp. 211 - 212
Copyright
Copyright © Astronomical Society of Australia 1969

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References

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