We investigate the effects of active galactic nucleus (AGN) feedback on the colour evolution of galaxies found in local (z < 0.2) groups and clusters. Galaxies located within the lobes of powerful Fanaroff-Riley type II (FR II) (edge-brightened) sources show much redder colours than neighbouring galaxies that are not spatially coincident with the radio source. By contrast, no similar effect is seen near FR I (core-dominated) radio sources. We show that these colours are consistent with FR II sources truncating star formation as the expanding bow shock overruns a galaxy. We examine a sample of clusters with no detectable radio emission and show that galaxy colours in these clusters carry an imprint of past AGN feedback. The AGN activity in t...
Several lines of argument support the existence of a link between activity at the nuclei of galaxies...
We explore the processes that trigger local AGN and the role of these AGN in regulating star formati...
International audienceContext. Several problems with the process of galaxy formation are still open....
We investigate the effects of active galactic nucleus (AGN) feedback on the colour evolution of gala...
The effects of active galactic nucleus (AGN) feedback on group and cluster galaxies are investigated...
Aim: The project address the relation between star formation and AGN activity in a large sample of n...
Feedback, in particular from active galactic nuclei (AGNs), is believed to play a crucial role in th...
Simulations of galaxy growth need to invoke strong negative feedback from active galactic nuclei (AG...
The effect of active galactic nuclei (AGN) on their host galaxies – in particular their levels of st...
International audienceThe relationship between galaxies of intermediate stellar mass and moderate lu...
Context. The discovery of the M − σ relation, the local galaxy bimodality, and the link between blac...
We study the effects of Active Galactic Nuclei (AGN) feedback on the formation and evolution of gala...
<p>The mechanism triggering the radio emission in Radio-Quiet (RQ) Active Galactic Nuclei (AGN), fou...
It has been speculated that low-luminosity radio-loud active galactic nuclei (AGN) have the potentia...
Active galactic nuclei (AGN) driven feedback has been proposed to be one of the most efficient ways ...
Several lines of argument support the existence of a link between activity at the nuclei of galaxies...
We explore the processes that trigger local AGN and the role of these AGN in regulating star formati...
International audienceContext. Several problems with the process of galaxy formation are still open....
We investigate the effects of active galactic nucleus (AGN) feedback on the colour evolution of gala...
The effects of active galactic nucleus (AGN) feedback on group and cluster galaxies are investigated...
Aim: The project address the relation between star formation and AGN activity in a large sample of n...
Feedback, in particular from active galactic nuclei (AGNs), is believed to play a crucial role in th...
Simulations of galaxy growth need to invoke strong negative feedback from active galactic nuclei (AG...
The effect of active galactic nuclei (AGN) on their host galaxies – in particular their levels of st...
International audienceThe relationship between galaxies of intermediate stellar mass and moderate lu...
Context. The discovery of the M − σ relation, the local galaxy bimodality, and the link between blac...
We study the effects of Active Galactic Nuclei (AGN) feedback on the formation and evolution of gala...
<p>The mechanism triggering the radio emission in Radio-Quiet (RQ) Active Galactic Nuclei (AGN), fou...
It has been speculated that low-luminosity radio-loud active galactic nuclei (AGN) have the potentia...
Active galactic nuclei (AGN) driven feedback has been proposed to be one of the most efficient ways ...
Several lines of argument support the existence of a link between activity at the nuclei of galaxies...
We explore the processes that trigger local AGN and the role of these AGN in regulating star formati...
International audienceContext. Several problems with the process of galaxy formation are still open....