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OH-IR Sources and the Galactic Centre Distance

Published online by Cambridge University Press:  23 September 2016

R. J. Cohen ,
M. Shepherd ,
M. J. Gaylard  and
M. E. West
R. J. Cohen
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, England
M. Shepherd
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, England
M. J. Gaylard
Affiliation:
Hartebeesthoek Radio Astronomy Observatory, P.O. Box 443, Krugersdorp 1740, South Africa
M. E. West
Affiliation:
Hartebeesthoek Radio Astronomy Observatory, P.O. Box 443, Krugersdorp 1740, South Africa

Abstract

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The phase-lag technique of estimating distance to OH-IR sources is briefly described. Preliminary results are presented from a study of nine OH-IR sources in the galactic centre direction.

Type
Perspectives
Information
Symposium - International Astronomical Union , Volume 136: The Galactic Center , 1989 , pp. 51 - 54
Copyright
Copyright © Kluwer 1989 

References

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