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Pressure-regulated star formation is a simple variant on the usualsupernova-regulated star formation efficiency that controls the global starformation rate as a function of cold gas content in star-forming galaxies, andaccounts for the Schmidt-Kennicutt law in both nearby and distant galaxies.Inclusion of AGN-induced pressure, by jets and/or winds that flow back onto agas-rich disk, can lead under some circumstances to significantly enhanced starformation rates, especially at high redshift and most likely followed by themore widely accepted phase of star formation quenching. Simple expressions arederived that relate supermassive black hole growth, star formation and outflowrates. The ratios of black hole to spheroid mass and of both black holeaccretion and outflow rates to star formation rate are predicted as a functionof time. I suggest various tests of the AGN-triggered star formationhypothesis.

Unleashing Positive Feedback: Linking the Rates of Star Formation, Supermassive Black Hole Accretion and Outflows in Distant Galaxies