Abstract
USING the 25-m radiotelescope at Dwingeloo, we have recently completed the initial stages of a large scale OH survey. The detailed results will be reported later. The survey is designed to yield an unbiased set of data for all four 18-cm lines of OH.
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References
Wilson, W. J., and Barrett, A. H., Astr. Astrophys., 17, 385 (1972).
Burton, W. B., Astr. Astrophys. Suppl. Ser., 2, 261 (1970).
Rougoor, G. W., and Oort, J. H., Proc. natn. Acad. Sci. U.S.A., 46, 1 (1960).
Thackeray, A. D., Observatory, 95, 100 (1975).
Caswell, J. L., IAU Symp., 60, 423 (1974).
Wallerstein, G., Astrophys. Lett., 15, 83 (1973).
Minkowski, R., Stars and Stellar Systems, V, 341 (University of Chicago Press, Chicago, London, 1965).
Sanders, R. H., and Lowinger, T., Astr. J., 77, 292 (1972).
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BAUD, B., HABING, H., MATTHEWS, H. et al. A very high velocity 1,612-MHz OH source near the galactic centre. Nature 258, 406–407 (1975). https://doi.org/10.1038/258406a0
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DOI: https://doi.org/10.1038/258406a0