# Galaxy And Mass Assembly (GAMA): 'No Smoking' zone for giant elliptical galaxies?

## TL;DR

This study reveals that the radio emission of massive galaxies varies with the dynamical state of their galaxy groups, with younger groups hosting more radio-loud brightest galaxies, impacting models of galaxy evolution.

## Contribution

It introduces a semi-analytic model linking galaxy group dynamics to radio emission, highlighting environmental effects on supermassive black hole activity.

## Key findings

- Radio luminosity of brightest galaxies depends on group dynamical state.
- Higher fraction of radio-loud galaxies in dynamically young groups.
- Model reproduces observed dependence of radio emission on environment.

## Abstract

We study the radio emission of the most massive galaxies in a sample of dynamically relaxed and un-relaxed galaxy groups from Galaxy and Mass Assembly (GAMA). The dynamical state of the group is defined by the stellar dominance of the brightest group galaxy, e.g. the luminosity gap between the two most luminous members, and the offset between the position of the brightest group galaxy and the luminosity centroid of the group. We find that the radio luminosity of the most massive galaxy in the group strongly depends on its environment, such that the brightest group galaxies in dynamically young (evolving) groups are an order of magnitude more luminous in the radio than those with a similar stellar mass but residing in dynamically old (relaxed) groups. This observation has been successfully reproduced by a newly developed semi-analytic model which allows us to explore the various causes of these findings. We find that the fraction of radio loud brightest group galaxies in the observed dynamically young groups is ~2 times that in the dynamically old groups. We discuss the implications of this observational constraint on the central galaxy properties in the context of galaxy mergers and the super-massive blackhole accretion rate.