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A Slower Superluminal Velocity for the Quasar 1156+295

  • Authors: B. Glenn Piner and Kerry A. Kingham

Piner & Kingham 1997 The Astrophysical Journal Letters 485 L61.

  • Provider: AAS Journals

Caption: Fig. 2.

Motion of components in 1156+295. The vertical axis shows the separation in milliarcseconds of the center of the component from the presumed core. Component positions measured at 2 GHz are plotted as squares, and positions measured at 8 GHz are plotted as diamonds. The solid lines represent the best fit of the 2 GHz positions to motion with constant velocity, and the dotted lines represent the same fits for the 8 GHz positions.

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