Radiation, winds, and jets from the active nucleus of a massive galaxy can interact with its
interstellar medium, and this can lead to ejection or heating of the gas. This terminates star …

The assembly of stellar and supermassive black hole (SMBH) mass in elliptical galaxies
since z∼ 1 can help to diagnose the origins of locally observed correlations between SMBH …

Most theoretical models invoke quasar-driven outflows to quench star formation in massive
galaxies, and this feedback mechanism is required to account for the population of old and …

Quasar-mode Feedback in Nearby Type 1 Quasars: Ubiquitous Kiloparsec-scale Outflows and
Correlations with Black Hole Properties - IOPscience This site uses cookies. By continuing to …

We explore the multiwavelength properties of AGN host galaxies for different classes of
radio-selected AGN out to z≲ 6 via a multiwavelength analysis of about 7700 radio sources …

We examine the detailed physics of the feedback mechanism by relativistic active galactic
nucleus (AGN) jets interacting with a two-phase fractal interstellar medium (ISM) in the kpc …

The shutdown of star formation in galaxies is generally termed" quenching." Quenching may
occur through a variety of processes, eg, active galactic nucleus (AGN) feedback, stellar …

ABSTRACT We present the Spitzer Extragalactic Representative Volume Survey (SERVS),
an 18 deg 2 medium-deep survey at 3.6 and 4.5 μm with the postcryogenic Spitzer Space …

We report on the energetics of molecular outflows in 14 local ultraluminous infrared galaxies
(ULIRGs) that show unambiguous outflow signatures (P Cygni profiles or high-velocity …

The observed massive end of the galaxy stellar mass function is steeper than its predicted
dark matter halo counterpart in the standard Λ cold dark matter paradigm. In this paper, we …