Fig. 4.
Spectra of all molecular gas lines and continuum emission detected in the ALMA data of the program 2013.1.00180.S. Left: spectra of the entire galaxy. Right: spectra of the nuclear pixel. The dashed line in CO(3−2) spectrum corresponds to the frequency at which the stitching of the data of the two spectral windows, in which the continuum level and slope are not known with sufficient accuracy for the determination of the presence of a wind, took place.
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