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We study Red Misfits, a population of red, star-forming galaxies in the localUniverse. We classify galaxies based on inclination-corrected optical coloursand specific star formation rates derived from the Sloan Digital Sky SurveyData Release 7. Although the majority of blue galaxies are star-forming andmost red galaxies exhibit little to no ongoing star formation, a small butsignificant population of galaxies ($\sim$11 per cent at all stellar masses)are classified as red in colour yet actively star-forming. We explore a numberof properties of these galaxies and demonstrate that Red Misfits are not simplydusty or highly-inclined blue cloud galaxies or quiescent red galaxies withpoorly-constrained star formation. The proportion of Red Misfits is nearlyindependent of environment and this population exhibits both intermediatemorphologies and an enhanced likelihood of hosting an AGN. We conclude that RedMisfits are a transition population, gradually quenching on their way to thered sequence and this quenching is dominated by internal processes rather thanenvironmentally-driven processes. We discuss the connection between Red Misfitsand other transition galaxy populations, namely S0's, red spirals and greenvalley galaxies.

Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies