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High Resolution Spectra of M and C Stars by Fourier Transform Spectroscopy

Published online by Cambridge University Press:  30 March 2016

J. P. Maillard
J. P. Maillard*
Affiliation:
Laboratoire Aimé Cotton, C.N.R.S. II, Orsay, France

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A Michelson interferometer was put into operation during the year 1972 at the Coudé focus of the Haute-Provence Observatory’s 76-in. telescope. We built this instrument at Aimé Cotton Laboratory (Orsay-France) where the method of Fourier Transform Spectroscopy has been largely developed in the direction of very high resolution work. A complete description of this device has been given elsewhere (Guelachvili and Maillard, 1970) and further details on the present study are reported by Maillard (1973).

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