The definitive version is available at www.blackwell-synergy.com. Copyright Blackwell PublishingA major amendment in recent models of hierarchical galaxy formation is the inclusion of so-called active galactic nucleus (AGN) feedback. The energy input from an active central massive black hole is invoked to suppress star formation in early-type galaxies at later epochs. A major problem is that this process is poorly understood, and compelling observational evidence for its mere existence is still missing. In search for signatures of AGN feedback, we have compiled a sample of 16 000 early-type galaxies in the redshift range 0.05 200 km s ) and roughly evenly distributed between star formation and AGN at intermediate and low (σ <100 km s ) mas...
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
We exploit a sample of 80 000 Sloan Digital Sky Survey central galaxies to investigate the effect of...
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution of gala...
The mechanisms for quenching star formation in galaxies are not yet well understood. Identifying the...
The mechanisms for quenching star formation in galaxies are not yet well understood. Identifying the...
We study stellar assembly and feedback from active galactic nuclei (AGN) around the epoch of peak st...
We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution of gala...
We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution of gala...
How galaxies maintain the inefficiency of star formation with physically self-consistent models is a...
How galaxies maintain the inefficiency of star formation with physically self-consistent models is a...
Recent work (Schawinski et al.) indicates that star-forming early-type galaxies residing in the blue...
We investigate radio-mode AGN activity among post-starburst galaxies from the Sloan Digital Sky Surv...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
We exploit a sample of 80 000 Sloan Digital Sky Survey central galaxies to investigate the effect of...
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution of gala...
The mechanisms for quenching star formation in galaxies are not yet well understood. Identifying the...
The mechanisms for quenching star formation in galaxies are not yet well understood. Identifying the...
We study stellar assembly and feedback from active galactic nuclei (AGN) around the epoch of peak st...
We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution of gala...
We study the effects of active galactic nuclei (AGN) feedback on the formation and evolution of gala...
How galaxies maintain the inefficiency of star formation with physically self-consistent models is a...
How galaxies maintain the inefficiency of star formation with physically self-consistent models is a...
Recent work (Schawinski et al.) indicates that star-forming early-type galaxies residing in the blue...
We investigate radio-mode AGN activity among post-starburst galaxies from the Sloan Digital Sky Surv...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...
We exploit a sample of 80 000 Sloan Digital Sky Survey central galaxies to investigate the effect of...
Residual star formation at late times in early-type galaxies and their progenitors must be suppresse...