Optical diameters of stars measured with the Mt. Wilson Mark III interferometer

Details Optical diameters of stars measured with the Mt. Wilson Mark III interferometer Optical diameters of stars measured with the Mt. Wilson Mark III interferometer

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990spie.1237..316s&link_type=abstract

IN: Amplitude and intensity spatial interferometry; Proceedings of the Meeting, Tucson, AZ, Feb. 14-16, 1990 (A91-30676 12-89).

Physics

Diameters, Giant Stars, Main Sequence Stars, Michelson Interferometers, Calibrating, Dimensional Measurement, Limb Darkening, Optical Measuring Instruments

Scientific paper

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.

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