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The Detection of Stellar Systems by Lunar Occultations

Published online by Cambridge University Press:  12 April 2016

N. M. White
N. M. White*
Affiliation:
Lowell Observatory, Flagstaff, Arizona

Abstract

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A few examples of the resolution of very close multiple stars by the method of lunar occultation are described. In this way both the power and some of the limitations of this technique may be demonstrated.

Resumen

Resumen

Se describen algunos ejemplos de la resolución de estrellas múltiples muy cercanas, mediante el método de ocultaciones lunares. De esta manera se muestran tanto el poder, como algunas de las limitaciones de esta técnica.

Type
Session 1
Information
International Astronomical Union Colloquium , Volume 33: Observational Parameters and Dynamical Evolution of Multiple Stars , May 1977 , pp. 43 - 46
Copyright
Copyright © Otto G. Franz and Paris Pismis 1977

References

Cowley, A., Cowley, C., Jaschek, M., and Jaschek, C. 1969, A.J., 74, 375.CrossRefGoogle Scholar
Finsen, W. S., and Worley, C. E. 1970, Republ. Obs. Johannesb. Circ, 7, No. 129.Google Scholar
Hoffleit, D. 1964, Catalogue of Bright Stars (Yale University: New Haven).Google Scholar
MacMahon, P. A. 1909, M.N.R.A.S., 69, 126.CrossRefGoogle Scholar