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A 28kHz-Resolution Acousto-Optic Spectrometer

Published online by Cambridge University Press:  04 August 2017

J-S. Wang ,
B.J. Robinson ,
G-C. Huang  and
R.E. Otrupcek
J-S. Wang
Affiliation:
Yunnan Observatory, Academia Sinica, P.O. Box 110, Kunming, China
B.J. Robinson
Affiliation:
Radiophysics, CSIRO, P.O. Box 76, Epping, NSW 2121, Astralia
G-C. Huang
Affiliation:
Shanghia Inst. of Ceramics, 865 Changning Road, Shanghai, China
R.E. Otrupcek
Affiliation:
Radiophysics, CSIRO, P.O. Box 76, Epping, NSW 2121, Astralia

Abstract

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A 28kHz resolution acousto-optic spectrometer has been established. The modulator is a TeO2 cell with off-axis acoustic slow shear wave. The convolution between the profiles of the modulator and the photodiode array was considered. Its velocity resolution is 0.07 kms−1 for 115 GHz CO molecular lines. The test observations were made by association with the 4-m mm-wave telescope in Australia. Some features of the CO lines in dark clouds have been seen more in detail.

Type
Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 135 - 136
Copyright
Copyright © Reidel 1987 

References

Cole, T.W., and Ables, J.G.: 1974, Astron. Astrophys. 34, 149.Google Scholar
Kaifu, N., Ukita, N., Chikada, Y., and Miyaji, T.: 1977, Publ. Astron. Soc. Japan 29, 429.Google Scholar
Malkamäki, L.J.: 1981, Astron. Astrophys. 98, 15.Google Scholar
Robinson, B.J.: 1980, IAU Symp. No. 87, 619.CrossRefGoogle Scholar
Winnewisser, G., and Vowinkel, B.: 1984, Sonderdruck aus Sterne und Weltraum 23, Seite 132.Google Scholar