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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 4.

Variation of the CSO radio power vs. the hotspot separation velocity. As a group, the sources with higher v HS generally have a higher radio power P rad and also a higher source power P src. Individual sources are predicted to evolve from high- v HS and low- P rad to low- v HS and high- P rad with time as P radv −1 HS. Symbols indicate high-power (circles) and low-power (squares) CSOs. Arrows on the symbols indicate upper limits.

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