Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2025-01-05T16:48:59.506Z Has data issue: false hasContentIssue false
  • English
  • Français

An attempt to detect the 327-Mc/s line of galactic deuterium

Published online by Cambridge University Press:  14 August 2015

R. L. Adgie
R. L. Adgie*
Affiliation:
Royal Radar Establishment, Malvern, England

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The previous unsuccessful attempts to detect the 327-Mc/s line of galactic deuterium [1, 2] were limited in sensitivity either by the size of aerial or by the inability to use long integration times with a large fixed aerial. The new observations reported here were made with the 250-foot radio telescope at Jodrell Bank, which can continuously follow a source of radiation; moreover, the effective integration time was improved by using a multi-channel receiver instead of a swept-frequency one.

Type
Part III: Galactic and Extragalactic Radio Sources
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 352 - 354
Copyright
Copyright © Stanford University Press 1959 

References

1. Adgie, R. L., and Hey, J. S. Nature , 179, 370, 1957.CrossRefGoogle Scholar
2. Stanley, G. J., and Price, R. Nature , 177, 1221, 1956.CrossRefGoogle Scholar
3. McClain, E. F. Ap. J. 122, 376, 1955.CrossRefGoogle Scholar
4. Hagen, J. P., Lilley, A. E., and McClain, E. F. Ap. J. 122, 361, 1955.CrossRefGoogle Scholar
5. Muller, C. A. Ap. J. 125, 830, 1957.CrossRefGoogle Scholar
6. van Woerden, H., Rougoor, G. W., and Oort, J. H. C.R. 244, 1691, 1957.Google Scholar
7. Suess, H. E., and Urey, H. C. Rev. Mod. Phys. 28, 53, 1956.CrossRefGoogle Scholar