Linked from

The 13 pages that link to Active galactic nucleus feedback, each with the reason it gives.

• Elliptical galaxyRelated: Feedback can heat or expel gas, helping suppress star formation in massive ellipticals.

• Galaxy evolutionRelated: It can heat or expel gas that would otherwise form stars.

• Galaxy formation and evolutionRelated: It can heat or expel gas, helping explain why massive galaxies stop forming stars.

• Intracluster mediumRelated: Energy from cluster galaxies can heat the gas and offset radiative cooling.

• Galaxy quenchingRelated: Energy from an active nucleus can heat or expel gas that would otherwise form stars.

• Radio galaxyRelated: Radio jets heat and disturb gas, regulating cooling and star formation in and around the host.

• Galaxy groupRelated: Feedback can heat group gas and regulate the cooling that feeds new stars.

• Galaxy luminosity functionRelated: It can suppress bright-end galaxy growth and shape the abundance of luminous systems.

• Luminous infrared galaxyRelated: Infrared observations help assess whether accretion-driven outflows regulate star formation.

• Perseus ClusterRelated: Feedback from NGC 1275’s nucleus heats the gas and helps regulate cooling.

• Brightest cluster galaxyRelated: Jets from the central galaxy can heat cluster gas and suppress continued cooling.

• cD galaxyRelated: Feedback from cD nuclei can heat cluster gas and regulate cooling near the cluster center.