Radio Brightness Contours of 3C273

Details Radio Brightness Contours of 3C273 Radio Brightness Contours of 3C273

Jul 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965natur.207..178h&link_type=abstract

Nature, Volume 207, Issue 4993, pp. 178-179 (1965).

Computer Science

8

Scientific paper

PREVIOUS observations of the radio source 3C273 by the method of lunar occultations have shown that it consists of two separate components the positions of which were determined with an accuracy of 1 arc sec1. Component A coincides closely with a jet-like nebulosity and component B with a nearby object of stellar appearance2. This communication presents a contour map of the source, constructed from the analysis of five complete occultations.

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