Feedback in Galaxy Formation

Details Feedback in Galaxy Formation Feedback in Galaxy Formation

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..339s&link_type=abstract

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S

Physics

Scientific paper

The physics of forming galaxies constrains their evolution in a highly nonlinear way. Observational phenomenology motivates the need for negative feedback to operate via supernova explosions in disk galaxies and via AGN outflows for quenching star formation in massive early-type galaxies. AGN-triggered and supernova-enhanced positive feedback may also be required to account both for ultra-luminous infrared galaxies and the presence of extremely red galaxies at high redshift.

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