The Lockman–SpReSO project - Galactic flows in a sample of far-infrared galaxies

Open Access

Fig. 7.

Weighted EW average of the Fe II lines versus M_*, SFR, and sSFR (from left to right). The empty blue circles are the results of this paper and the empty orange diamonds are the results of PR21. The inset plots represent the same idea as in Fig. 5. See the Sect. 4.1 for a discussion of correlation.

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