Fig. 5.
[O I]63 μm fine structure lines of LARS galaxies, obtained with Herschel/PACS. Total fluxes were derived using Gaussian fits (see Table 6). The zero-velocity (red vertical line) is related to the H I systemic velocity from Pardy et al. (2014) for all LARS galaxies except LARS 12−14 (which have no H I detection). For those, the systemic velocity is based on SDSS optical redshifts.
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