Fig. 1.

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Left panel: radial shock velocity (vs, violet) and axial position (black) for jet powers 1046 (solid lines), 1044 (dashed), and 1042 erg s−1 (dotted). The thin, dark red lines indicate the ISM sound speed at the axial position. Right panel: post-shock temperatures for same jet powers as the left panel in the case of a medium density following Eq. (7) (black lines), i.e., a hot, diffuse ISM, and a medium with constant number density 103 cm−3, i.e., cold clouds. Horizontal lines indicate hydrogen ionization temperatures in local thermodynamical equilibrium, 3500 K (solid), and collisional equilibrium, 1.58 × 105 K (dashed). In these clouds, the sound speed is 3 km s−1. The temperatures have been derived for ionized hydrogen in Eq. (10).
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