Dopita, MichaelGroves, BrentSutherland, RalphKewley, Lisa2015-12-130004-637Xhttp://hdl.handle.net/1885/86841Star formation rates in galaxies are frequently estimated using the Balmer line fluxes of their H II regions. However, these can be systematically underestimated because dust competes for the absorption of Lyman continuum photons in the ionized gas. ThisKeywords: Dust, extinction; Galaxies: starburst; H II regions; Stars: formationInternal Dust Correction Factors for Star Formation Rates Derived for Dusty HII Regions and Starburst Galaxies200310.1086/3454482015-12-12