Shocks, clouds, and atomic outflows in active galactic nuclei hosting relativistic jets

Open Access

Fig. 2.

Lobe overpressure for jet powers 10⁴⁶ (solid lines), 10⁴⁴ (dashed), and 10⁴² erg s⁻¹. The black lines for the hot, diffuse ISM, and red lines correspond to cold, dense clouds with a number density of 10³ cm⁻³ are overlapped.

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