Abstract
AFTER the radioastronomical detection1 of helium in 1966 a programme to study the 109α transition of neutral helium was begun at the US National Radio Astronomy Observatory, and helium has now been detected in five sources (as will be described elsewhere). During the course of this work, however, unidentified microwave spectral emission has also been detected in the sources NGC 2024 and IC 1795. This communication describes the observed physical characteristics of this emission, considers its possible origins and suggests further observations to identify it. In the succeeding communication, Goldberg and Dupree argue that the new line is a recombination line of carbon I.
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References
Lilley, A. E., Palmer, P., Penfield, H., and Zuckerman, B., Nature, 211, 174 (1966).
Zuckerman, B., Palmer, P., Penfield, H., and Lilley, A. E., Astrophys. J. (in the press).
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PALMER, P., ZUCKERMAN, B., PENFIELD, H. et al. Detection of a New Microwave Spectral Line. Nature 215, 40–41 (1967). https://doi.org/10.1038/215040a0
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DOI: https://doi.org/10.1038/215040a0
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