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Stellar Multiplicity Discovery by Lunar Occultations

Published online by Cambridge University Press:  12 April 2016

Nathaniel M. White
Nathaniel M. White*
Affiliation:
Lowell Observatory, Flagstaff, AZ, USA

Abstract

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The primary result of lunar occultation studies of multiple star systems is the discovery of new systems. Its use as a method of multiplicity discovery has been productive, although incidental to timing observations made by amateurs and professionals for 360 years. The capabilities and limitations as a method of discovering new double stars is discussed.

Type
High Resolution At Visual Wavelengths
Information
International Astronomical Union Colloquium , Volume 135: Complementary Approaches to Double and Multiple Star Research , 1992 , pp. 486 - 491
Copyright
Copyright © Astronomical Society of the Pacific 1992

References

Appleby, G.M. 1980, J. Brit. Astron. Assoc., 90, 572 Google Scholar
Evans, D. 1970, AJ, 75, 589 Google Scholar
Evans, D.S. 1983, in Current Techniques in Double and Multiple Star Research, IAU Colloquium No. 62, Lowell Obs. Bull., No. 167 Google Scholar
Nather, R.E. & Evans, D. 1970, AJ, 75, 575 Google Scholar
Nather, R.E. & McCants, M.M. 1970, AJ, 75, 963 Google Scholar
Shara, M.M., Doxsey, R., Wells, E.N., & McAlister, H.A. 1987, PASP, 99, 223 Google Scholar
Warner, B. 1988, High Speed Astronomical Photometry, (Cambridge University Press)Google Scholar