1 August 1990 Optical diameters of stars measured with the Mt. Wilson Mark III interferometer
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Abstract
Reliable stellar angular diameters can now be determined using the Mark III Optical Interferometer located on Mt. Wilson, California. The Mark III is a Michelson Interferometer capable of measuring the interferometric fringe visibility for stars using interferometer baselines varying from 3 to 31.5 meters in length. Angular diameters measured with the Mark III Optical Interferometer are presented for 12 stars at wavelengths of 450 and 800 nm.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Richard S. Simon, Richard S. Simon, David Mozurkewich, David Mozurkewich, Kenneth J. Johnston, Kenneth J. Johnston, Ralph Gaume, Ralph Gaume, Donald J. Hutter, Donald J. Hutter, P. F. Bowers, P. F. Bowers, M. Mark Colavita, M. Mark Colavita, Michael Shao, Michael Shao, } "Optical diameters of stars measured with the Mt. Wilson Mark III interferometer", Proc. SPIE 1237, Amplitude and Intensity Spatial Interferometry, (1 August 1990); doi: 10.1117/12.19304; https://doi.org/10.1117/12.19304
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