Abstract
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.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
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.
Elitzur, M., 1982. Rev.Mod.Phys., 54, 1225–1260.
Feast, M., 1987. “The Galaxy”, pp 1–25, eds. Gilmore, G. & Carswell, R., Reidel, Dordrecht, Holland.
Goldreich, P. & Scoville, N.Z., 1976. Astrophys.J., 205, 144–154.
Herman, J., 1983. Ph.D. Thesis, University of Leiden.
Huggins, P.J. & Glassgold, A.E., 1982. Astr.J., 87, 1828–1835.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1989 IAU
About this paper
Cite this paper
Cohen, R.J., Shepherd, M., Gaylard, M.J., West, M.E. (1989). OH-IR Sources and the Galactic Centre Distance. In: Morris, M. (eds) The Center of the Galaxy. International Astronomical Union Union Astronomique Internationale, vol 136. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2362-1_5
Download citation
DOI: https://doi.org/10.1007/978-94-009-2362-1_5
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-0222-3
Online ISBN: 978-94-009-2362-1
eBook Packages: Springer Book Archive