High Resolution Spectra of M and C Stars by Fourier Transform Spectroscopy
- 1 January 1974
- journal article
- other
- Published by Cambridge University Press (CUP) in Highlights of Astronomy
- Vol. 3, 269-284
- https://doi.org/10.1017/s1539299600001982
Abstract
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).Keywords
This publication has 1 reference indexed in Scilit:
- The Infrared Spectrum of Alpha Herculis from 4000 to 4800 cm^{-1}Publications of the Astronomical Society of the Pacific, 1972