Fig. 9
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Properties of the hot wind predicted by our best-fit models (in red; see main text for more details), compared to recent X-ray observational constraints from XMM-Newton (Ponti et al. 2019). From top to bottom, hot gas velocity, density, and temperature. The dashed curves show the predictions for a model where the hot mass loading factor ηM is forced to values close to 1 (see Section 5.1.1).
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