Fig. 4 from Sub‐Milliarcsecond Precision of Pulsar Motions: Using In‐Beam Calibrators with the VLBA

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Sub‐Milliarcsecond Precision of Pulsar Motions: Using In‐Beam Calibrators with the VLBA

Authors: E. B. Fomalont, W. M. Goss, A. J. Beasley, and S. Chatterjee

Fomalont et al. 1999 The Astronomical Journal 117 3025.

Provider: AAS Journals

Caption: Fig. 4.

Residual motion of pulsar B0919+06, as comparison of the measured east‐west position of the pulsar following removal of the best‐fit east‐west position and proper motion listed in the plot. The sinusoid corresponds to the residual motion expected for a source with parallax 0.31 mas.

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