Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-26T14:47:09.640Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Diamond, P.J., Norris, R.P., Rowland, P.R., Booth, R.S. & Nyman, L-A., 1985. Mon. Not. R. astr. Soc., 212, 1–21.Google Scholar
Elitzur, M., 1982. Rev. Mod. Phys., 54, 1225–1260.Google Scholar
Feast, M., 1987. “The Galaxy”, pp1–25, eds. Gilmore, G. & Carswell, R., Reidel, Dordrecht, Holland.Google Scholar
Goldreich, P. & Scoville, N.Z., 1976. Astrophys. J., 205, 144–154.Google Scholar
Herman, J., 1983. Ph.D. Thesis, University of Leiden.Google Scholar
Huggins, P.J. & Glassgold, A.E., 1982. Astr. J., 87, 1828–1835.CrossRefGoogle Scholar