HI-deficient perturbed galaxies show steeper faint-end slopes in HII region luminosity functions, brighter characteristic luminosities, and fewer HII regions per unit stellar mass and disk area than unperturbed systems, with the effect strongest in outer disks.
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A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). XXI. Statistical properties of individual HII regions in perturbed galaxies
HI-deficient perturbed galaxies show steeper faint-end slopes in HII region luminosity functions, brighter characteristic luminosities, and fewer HII regions per unit stellar mass and disk area than unperturbed systems, with the effect strongest in outer disks.