Properties of the HII Regions Derived Using Integral Field Spectroscopy
Figure 2
(a) Absolute value of the equivalent width of H, in logarithmic scale, plotted against the luminosity fraction of young stars in the -band, in the underlying stellar population (according to the SSP modelling by FIT3D) for the clumpy ionized regions selected with HIIEXPLORER. (b) Absolute value of the equivalent width of H, in logarithmic scale, plotted against the oxygen abundance for the same ionized regions. (c) Absolute value of the equivalent width of H, in logarithm scale, plotted against the ionization strength for the same ionized regions.
