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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).

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 3: Highlights of Astronomy. As presented at the XVth General Assembly of the IAU, 1973 , 1974 , pp. 269 - 284
Copyright
Copyright © Reidel 1974

References

Boyce, P. B. and Sinton, W. M.: 1964, Astron. J. 69, 534.Google Scholar
Chauville, J., Querci, F., Connes, J., and Connes, P.: 1970, Astron. Astrophys. Suppl. 2, 181.Google Scholar
Connes, J., Connes, P., and Maillard, J.-P.: 1967, Coll. ‘Méthodes Nouvelles de Spectroscopie Instrumentale’, J. Phys. 28, C2.Google Scholar
(English transl, in New Methods in Instrumental Spectroscopy, Gordon and Breach, 1972).Google Scholar
Cormes, J., Connes, P., Bouigue, R., Querci, F., Chauville, J., and Querci, M.: 1968, Ann. Astrophys 31, 485.Google Scholar
Frogel, J. and Hyland, A.: 1972, Mem. Soc. Roy. Sci. Liège, 6th Ser. 3, 111.Google Scholar
Fujita, Y.: 1970, Interpretation of Spectra and Atmospheric Structure in Cool Stars, Univeristy Park Press.Google Scholar
Guelachvili, G. and Maillard, J.-P.: 1970, Aspen International Conference on Fourier Spectroscopy. AFCRL Special Report No. 114, p. 151.Google Scholar
Johnson, H. L.: 1964, Bol. Obs. Tonantzintla Tacubaya 3, 305.Google Scholar
Johnson, H. L., Coleman, J., Mitchell, R. J., and Steinmetz, D. L.: 1968, Comm. Lunar Planetary Lab. 7, 83.Google Scholar
Kunde, V. G.: 1967, ‘Tables of Theoretical Line Positions and Intensities of the Δυ =1, Αυ = 2,Δυ =3 Vibration-Rotation Bands of CO’, NASA, X-622-67-248.Google Scholar
Lockwood, G. W. and Wing, R. F.: 1971, Astrophys. J. 169, 63.Google Scholar
Maillard, J.-P.: 1973, Thèse d’Etat, Université de Paris-Sud, No. 1157.Google Scholar
Mantz, A. W., Nichols, F. R., Alpert, B. D., and Rao, V. N.: 1970, J. Mol. Spectrosc. 35, 325.Google Scholar
McCammon, D., Münch, G., and Neugebauer, G.: 1967, Astrophys. J. 147, 575.Google Scholar
Mertz, L.: 1972, Mem. Soc. Roy. Sci. Liège, 6th Ser. 3, 101.Google Scholar
Neugebauer, G. and Leighton, R.: 1969, ‘Two-Micron Sky Survey - Preliminary Catalog’, Caltech, Pasadena, Cal., NASA, Washington, D.C. Google Scholar
Querci, F.: 1974, this volume, p. 341.Google Scholar
Thompson, R. I., Johnson, H. L., Forbes, F. F., and Steinmetz, D. L.: 1972, Publ. Astron. Soc. Pacific 84, 775 and 779.Google Scholar
Wilson, R. E.: 1953, General Catalogue of Stellar Radial Velocities, Carnegi e Institution of Washington, Washington, D.C., Pub. No. 601.Google Scholar