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1612 MHz observations of southern IRAS sources

Published online by Cambridge University Press:  04 August 2017

M. E. Dollery ,
M. J. Gaylard  and
R. J. Cohen
M. E. Dollery
Affiliation:
Hartebeesthoek Radio Astronomy Observatory
M. J. Gaylard
Affiliation:
Hartebeesthoek Radio Astronomy Observatory
R. J. Cohen
Affiliation:
University of Manchester, Nuffield Radio Astronomy Labs., Jodrell Bank

Abstract

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Eight of thirty-four previously unobserved IRAS sources were found to be relatively strong 1612 MHz OH emitters. Five of these emit at 1667 MHz. Of the eight half are high velocity range, population I type stars, the other half are low velocity range, population II type stars. The pump efficiencies are in the range 0.018 ≤ e ≤ 0.163.

Type
Circumstellar Shells and Envelopes
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 215 - 216
Copyright
Copyright © Reidel 1987 

References

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