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White, Glenn J. and Ricketts, Martin J.
(1979).
DOI: https://doi.org/10.1093/mnras/187.4.757
URL: http://adsabs.harvard.edu/abs/1979MNRAS.187..757W
Abstract
Observations of the quasar 3C273 made during 1975-77 have shown that the X-ray flux varied on a time scale of several months. No similar variation was present in radio and optical data taken at similar times. If this variation results from luminosity variations of a central compact object, then an upper limit of ≤4 x 1017cm can be set on its dimensions.