The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end

TL;DR

This paper explains how hot gas haloes in massive galaxies suppress star formation and promote black hole growth, leading to the transition from blue to red galaxy sequences, supported by an analytic model and simulations.

Contribution

It introduces a simple analytic model linking hot haloes, star formation-driven outflows, and black hole activity to galaxy evolution, validated by hydrodynamic simulations.

Findings

Galaxies below 3×10^{10} M_\odotalance star formation and outflows.

Above 10^{12} M_\odot he hot corona triggers black hole growth and star formation cessation.

Transition mass scale is stable with star formation outflows, absent outflows eliminate the transition.

Abstract

Galaxies fall into two clearly distinct types: `blue-sequence' galaxies that are rapidly forming young stars, and `red-sequence' galaxies in which star formation has almost completely ceased. Most galaxies more massive than $3\times10^{10} M_\odot$ follow the red-sequence while less massive central galaxies lie on the blue sequence. We show that these sequences are created by a competition between star formation-driven outflows and gas accretion on to the supermassive black hole at the galaxy's center. We develop a simple analytic model for this interaction. In galaxies less massive than $3\times10^{10} M_\odot$, young stars and supernovae drive a high entropy outflow that is more buoyant that any diffuse corona. The outflow balances the rate of gas inflow, preventing high gas densities building up in the central regions. More massive galaxies, however, are surrounded by a hot corona. We argue that above a halo mass of $\sim 10^{12} M_\odot$, the supernova-driven outflow is no longer buoyant and star formation is unable to prevent the build up of gas in the central regions. This triggers a strongly non-linear response from the black hole. Its accretion rate rises rapidly, heating the galaxy's corona, disrupting the incoming supply of cool gas and starving the galaxy of the fuel for star formation. The host galaxy makes a transition to the red sequence, and further growth predominantly occurs through galaxy mergers. We show that the analytic model provides a good description of galaxy evolution in the EAGLE hydrodynamic simulations, and demonstrate that, so long as star formation-driven outflows are present, the transition mass scale is almost independent of subgrid parameter choice. The transition mass disappears entirely, however, if star formation driven outflows are absent.