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The Dynamic Evolution of Young Extragalactic Radio Sources

  • Authors: Tao An and Willem A. Baan

An & Baan 2012 The Astrophysical Journal 760 77.

  • Provider: AAS Journals

Caption: Figure 7.

Variation of the linear size and the separation velocity with kinematic age. (a) Both source groups (high and low radio power) are consistent with hotspot separation velocity decreasing with age. The predicted evolution of the sources follows a v HST −2/5 kin relation (dashed arrows). (b) The CSO linear size shows an expected increase with age. The predicted variation for individual sources with constant power is DT 3/5 kin as indicated with dashed arrows. As a group the older sources also have larger sizes as DT 1.5 kin (dotted line).

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