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Measurement of the Microwave Background Temperature from CN Absorption

Published online by Cambridge University Press:  19 July 2016

N. Mandolesi
Affiliation:
Istituto TESRE-CNR, Via de' Castagnoli, 1, 40126 Bologna, Italy
P. Crane
Affiliation:
European Southern Observatory, Karl Schwarzschildstrasse, 2 D-8045 Garching, Western Germany
D.J. Hegyi
Affiliation:
Department of Physics, University of Michigan, Ann Arbor, Michigan USA

Abstract

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Observations of the interstellar lines of CN near 3875Å toward ζ Oph provide precise measurements of the Microwave Background Radiation (MBR) temperature and determine the intrinsic linewidth necessary for the saturation correction. We report TMBR=2.74±0.05 K at λ=2.64 mm and TMBR=2.75 (+0.24, −0.29) K at λ=1.32 mm.

Type
Chapter I: The Microwave Background Radiation
Copyright
Copyright © Reidel 1987 

References

Crane, P., Hegyi, D.J., Mandolesi, N., and Danks, A.C., 1986, Ap. J., 309.CrossRefGoogle Scholar
Hegyi, D.J., Traub, W., and Carleton, N.P., 1972, Phys Rev. Letters, 28, 1541.CrossRefGoogle Scholar
Mandolesi, N., Calzolari, P., Cortiglioni, S., Morigi, G., Danese, L., and De Zotti, G., 1986, Ap. J., 310.CrossRefGoogle Scholar
Meyer, D.M., and Jura, M., 1985, Ap. J., 297, 119.CrossRefGoogle Scholar
Morton, D.C., 1975, Ap. J., 197, 85.CrossRefGoogle Scholar
Smoot, G.F., De Amici, G., Friedman, S.D., Witebsky, C., Sironi, G. Bonelli, G., Mandolesi, N., Cortiglioni, S., Morigi, G. Partridge, R.B., Danese, L., and De Zotti, G., 1985, Ap. J. (Letters), 291, L23.CrossRefGoogle Scholar