Radio Emission from the Andromeda Nebula

Details Radio Emission from the Andromeda Nebula Radio Emission from the Andromeda Nebula

Aug 1954

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1954natur.174..320b&link_type=abstract

Nature, Volume 174, Issue 4424, pp. 320-321 (1954).

Physics

21

Scientific paper

OBSERVATIONS have been made at a wave-length of 3.7 m. with interferometers of different resolving powers to determine the distribution of radio brightness across the Andromeda nebula, M31, which has also been investigated at radio wave-lengths by Hanbury Brown and Hazard1. When observations are made with small movable aerials, errors are caused by reception of radiation from adjacent radio stars. Good discrimination was therefore obtained with the present measurements by using several different sections of the large Cambridge radio telescope2, although this method reduced the number of different axes and aerial spacings available. The relationship of the four axes used to the Andromeda nebula is shown in Fig. 1.

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