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The Nature and Evolution of Classical Double Radio Sources from Complete Samples

  • Authors: Katherine M. Blundell, Steve Rawlings, and Chris J. Willott

Blundell, Rawlings, & Willott 1999 The Astronomical Journal 117 677.

  • Provider: AAS Journals

Caption: Fig. 10.

Thick solid line, trajectory of a point moving out from the center of the AGN at which the break frequency has lowered to 1 GHz; thin solidline, the trajectory of one hotspot advancing away from the AGN; dashed line, the trajectory of the midpoint of the arm of a source (see text for more details). Trajectories are shown for a source whose jets each carry total kinetic energy Q0 = 1040 W (top) and Q0 = 5 × 1037 W (bottom). The value of φ was taken to be 5.

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