Intensity of the Radio Line of Galactic Deuterium

Details Intensity of the Radio Line of Galactic Deuterium Intensity of the Radio Line of Galactic Deuterium

Feb 1957

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1957natur.179..370a&link_type=abstract

Nature, Volume 179, Issue 4555, pp. 370-371 (1957).

Physics

2

Scientific paper

THE possibility of detecting deuterium in the galaxy by observation of a radio spectral line at a frequency of 327 Mc./s. has been discussed by Shklovsky1. He suggested that the line might be observable in absorption towards the galactic centre, a direction in which the background intensity of continuous radio emission is a maximum, and dispersion of the line by Doppler effect from galactic rotation is a minimum.

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