Variations of Small Quasar Components at 2,300 MHz

Details Variations of Small Quasar Components at 2,300 MHz Variations of Small Quasar Components at 2,300 MHz

Dec 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224.1094g&link_type=abstract

Nature, Volume 224, Issue 5224, pp. 1094-1095 (1969).

Computer Science

16

Scientific paper

IN a previous article1 we reported long-baseline interferometer measurements of several quasi-stellar radio sources using stations of the NASA/JPL Deep Space Network in Australia and California. Comparison of three sets of similar observations now shows evidence for secular variations in the apparent intensities of small-diameter components in several of these objects. The results are compatible with the theory of expanding synchrotron sources, but an apparent expansion velocity greater than that of light seems to be required for the recent outburst in 3C 273.

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