Observations of the Quasi-stellar and Other Radio Sources with an Interferometer of Resolving Power 0.4 sec of Arc

Details Observations of the Quasi-stellar and Other Radio Sources with an Interferometer of Resolving Power 0.4 sec of Arc Observations of the Quasi-stellar and Other Radio Sources with an Interferometer of Resolving Power 0.4 sec of Arc

Jan 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965natur.205..375a&link_type=abstract

Nature, Volume 205, Issue 4969, pp. 375-376 (1965).

Physics

36

Scientific paper

OBSBRVATIONS made previously at Jodrell Bank with long base-line interferometers1 have indicated that a small percentage of 384 sources examined with these interferometers have angular sizes of less than 1.0 sec of arc. Six were found to have fringe visibilities (γ) > 0.8 for transit observations with an east-west base-line of 61,100 wave-lengths.

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