Astrophysical Phenomena Revealed by Space VLBI
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We present results obtained from VLBI monitoring of the relativistic jet in 3C279 at 22 GHz from 1991 to 1997 (18 epochs), and at 43 GHz from 1995 to 1997 (10 epochs). Measured speeds for all detected components are presented. Component C4 has followed a nonlinear path out from the core, and the motion of this component is discussed in detail.
Piner, B. G., Wehrle, A. E., Unwin, S. C., Zook, A. C., Xu, W., & Marscher, A. P. (2000). VLBI Monitoring of 3C 279 at 22 and 43 GHz: 1991-1997. Astrophysical Phenomena Revealed by Space VLBI, 55. Retrieved from https://poetcommons.whittier.edu/phys/68