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The dependence of H ii region properties on global and local surface brightness within galaxy discs

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Figure

Figure 1. The ratio of the Hα flux (upper) and equivalent width (lower)to the observed Hα+[N II] flux for 12 262 star forming SDSS galaxies asmeasured by Tremonti et al
Figure 2. In the upper panel, the total extrapolated B-band magnitude (seeSection 2.1) for the 12 LSB galaxies observed at KPNO that are in the RC3catalogue versus the RC3 B-band magnitudes
Figure 3. The B-band central surface brightness (left-hand side) and B −R disc colours (right-hand side; see Section 2.1) distributions for the HSB(grey) and LSB (light grey) galaxies
Figure 5. The H II region LFs for the LSB galaxies observed at KPNO. LFs for galaxies with radial velocities <1000 km s−1 for which the distance estimatesare somewhat unreliable are highlighted in red.
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