The Quasar 3C309.1
Scott E. Aaron, John F.C. Wardle, & David H. Roberts

We have observed the quasar 3C309.1 at many frequencies between 1.4 and 43 GHz with the Very Long Baseline Array between 1995 and 1998, mapping the total intensity and linear polarization structure at angular resolution of the order of milliarcseconds.  The source is for the following reasons

Our observing projects allow us to examine and test all of these properties.  Our primary results are summarized below.
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