Fig. 13.
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Hα/Hβ ratio for the SDSS and GAMA sample for galaxies with varying inclination. Top two panels: inclination distribution, and the bottom two panels show the Hα/Hβ – inclination relation for the selected star-forming sample and the Hα/Hβ ratio – inclination relation from the T04 model with varying 
. We can see that none of the T04 models can describe the observed trend.
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