NASA NTRS · 19720039310
3C279 - Evidence for a non-superrelativistic model.
Abstract
Measurements of the observed variation of the total flux density of the quasi-stellar radio source 3C279 at 7.8 GHz are discussed. It is shown that these measurements are consistent with a model for 3C279 that does not involve an apparent source expansion rate of ten times the speed of light.
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Dent, W. A.. 1972-03-10. 3C279 - Evidence for a non-superrelativistic model.. https://ntrs.nasa.gov/citations/19720039310
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