Heating of the molecular gas in the massive outflow of the local ultraluminous-infrared and radio-loud galaxy 4C12.50

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Fig. 7

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Line profile of the main CO(1–0) emission component in the PdB data. The flux is integrated down to the 1σ level of the integrated CO(1–0) emission (Fig. 1; typically 7–9′′ from the radio core), excluding the emission from the tidal structure, which is shown in Fig. 8.

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