Regulation of star formation in giant galaxies by precipitation, feedback, and conduction

TL;DR

This paper explores how precipitation, feedback, and conduction regulate star formation in giant galaxies within clusters, emphasizing the role of thermal instability thresholds across different environments and cosmic times.

Contribution

It integrates observational evidence of cold gas thresholds with theoretical models to explain star formation regulation in galaxy clusters.

Findings

Precipitation threshold extends over large cluster ranges.

Cold gas abundance increases near the instability threshold.

Thermal conduction can suppress star formation by offsetting cooling.

Abstract

The universe's largest galaxies reside at the centers of galaxy clusters and are embedded in hot gas that, if left unchecked, would cool prodigiously and create many more new stars than are actually observed. Cooling can be regulated by feedback from accretion of cooling gas onto the central black hole, but requires an accretion rate finely tuned to the thermodynamic state of the hot gas. Theoretical models in which cold clouds precipitate out of the hot gas via thermal instability and accrete onto the black hole exhibit the necessary tuning. We have recently presented observational evidence showing that the abundance of cold gas in the central galaxy increases rapidly near the predicted threshold for instability. Here we present observations showing that this threshold extends over a large range in cluster radius, cluster mass, and cosmic time, and incorporate the precipitation threshold into a comprehensive framework of theoretical models for the thermodynamic state of hot gas in galaxy clusters. According to that framework, precipitation regulates star formation in some giant galaxies, while thermal conduction prevents star formation in others, if it can compensate for radiative cooling and shut off precipitation.