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Fig. 2.

Fig. 2. Refer to the following caption and surrounding text.

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H I emission column densities at the positions of the continuum sources plotted against continuum peak flux. The column densities are not corrected for inclination. Red triangles indicate detections. Circles indicate non-detections towards unresolved non-Hα sources, with filled symbols for i < 70° and open symbols for i ≥ 70°. Small stars indicate Hα star-forming regions, and small circles indicate resolved sources not associated with Hα. Filled circles mark the ‘clean’ sample of unresolved non-Hα sources in low-inclination galaxies. The horizontal dashed line shows the 3σ over 16 km s−1 column density limit of log(NH I/cm−2) = 19.77.

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