The Westerbork Coma Survey - A blind, deep, high-resolution H I survey of the Coma cluster

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Fig. 9.

Offsets from the star forming main sequence (as seen in Fig. 7) versus the gas fraction – stellar mass scaling relation (Fig. 8). The black line shows the best-fit linear relation for reference sample galaxies (Eq. (5)). Black errorbars are the mean uncertainties of the Coma measurements.

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