HIGHLIGHTS
- who: Francoise Combes from the University of Padua, Italy have published the paper: AGN Feedback and Its Quenching Efficiency, in the Journal: (JOURNAL)
SUMMARY
TYPES OF FEEDBACK Cosmological simulations in the CDM scenario predict too many galaxies at both ends of the mass function. A particular example of this feedback mode is the moderation of cooling flows in clusters, through radio-jets from the brightest central galaxy (BCG). The jets carve cavities in the ICM, and uplift some hot gas. In real clusters, gas cools in the border of cavities, which can occur . . .
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