Evolution of 3C 273 at 10.7 GHz

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Stellar Activity, Stellar Cores, Stellar Luminosity, Quasars, Stellar Evolution, Very Long Base Interferometry

Scientific paper

The quasar 3C 273 has been observed at 10.7 GHz at three epochs spanning 1984.1 to 1985.6. Two new superluminal components, C5 and C7a, are separating from the core with apparent transverse velocity V/c = (8.0 + or - 0.2)/h. The old components C3 and C4 may still be recognizable, with C4 having moved from 2.5 to perhaps 10 mas from the core in seven years. Non-monotonic curvature near the core is confirmed.

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