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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

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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

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