Extended Data Fig. 1: The impact of inclinations on the observed HI line width. | Nature

Extended Data Fig. 1: The impact of inclinations on the observed HI line width.

From: Black holes regulate cool gas accretion in massive galaxies

Extended Data Fig. 1

The relation between M and the observed HI line width are shown in panels (a, c), while the relation between M and the inclination-corrected HI line width are shown in panels(b, d), for MaNGA and xGASS galaxies respectively. The error bars refer to 1-σ errors for logM. For W50, we denote 20% measurement uncertainties.

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