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

Open Access

Fig. 3.

HI fraction in shocked clouds in LTE for jets with powers 10⁴⁴ (dashed), and 10⁴² erg s⁻¹ (dotted). The intermediate case of 10⁴³ erg s⁻¹ (dash-dot line) has been also included in this plot.

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