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Intensity of Low Frequency Recombination Lines

Published online by Cambridge University Press:  25 April 2016

M.J. Batty
M.J. Batty*
Affiliation:
School of Physics, University of Sydney
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Extract

Owing to the comparative lack of radio recombination line observations of southern HII regions, it has not been so far possible to make an overall interpretation of the data for these sources. However, observations of the H90α and H252α transitions by McGee et al. (1975) and Batty (1974) respectively have usefully extended the frequency range of observations to cover ∼ 0.4 to 8.9 GHz for a few southern HII regions.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 74 - 75
Copyright
Copyright © Astronomical Society of Australia 1976

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References

Batty, M. J., Mon.Not.Roy. Ast. Soc, 168, 37P (1974).CrossRefGoogle Scholar
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McGee, R. X., Newton, L. M., and Batchelor, R. A., Aust. J. Phys. 28, 185 (1975).CrossRefGoogle Scholar
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