Brightness Distribution of the Radio Source 14N5A

Details Brightness Distribution of the Radio Source 14N5A Brightness Distribution of the Radio Source 14N5A

Jul 1962

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1962natur.195..165a&link_type=abstract

Nature, Volume 195, Issue 4837, pp. 165-166 (1962).

Computer Science

18

Scientific paper

MANY radio sources are now known to have brightness distributions differing markedly from a radially symmetrical gaussian distribution1,2. Consequently the detailed investigation of individual radio sources by long baseline measurements has become particularly significant. The normal techniques which involve the moving of an outstation aerial to many sites at distances comparable with the maximum length of the baseline are difficult to apply with baselines of the order of 100 km. A further extension has therefore been made of the tracking technique3,4 in which the motion of the source across the sky is used to change the effective length of the baseline and its position angle relative to the source. This communication describes the investigation of the radio source 14N5A by this method. This source is of particular interest since it is the most distant source to be identified with an optical object.

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