An Evolutionary Paradigm for Dusty Active Galaxies at Low Redshift

TL;DR

This paper develops an evolutionary model for low-redshift infrared-luminous galaxies, revealing three phases of ULIRG development and identifying key spectral diagnostics for their lifecycle.

Contribution

It introduces a new evolutionary paradigm for ULIRGs based on Bayesian and graph theory methods, linking spectral features to galaxy development stages.

Findings

ULIRG lifecycle comprises three distinct phases.

The 11.2 micron PAH feature effectively indicates evolutionary stages.

Identification of six ULIRGs as archetypes of key lifecycle phases.

Abstract

We apply methods from Bayesian inferencing and graph theory to a dataset of 102 mid-infrared spectra, and archival data from the optical to the millimeter, to construct an evolutionary paradigm for z<0.4 infrared-luminous galaxies (ULIRGs). We propose that the ULIRG lifecycle consists of three phases. The first phase lasts from the initial encounter until approximately coalescence. It is characterized by homogeneous mid-IR spectral shapes, and IR emission mainly from star formation, with a contribution from an AGN in some cases. At the end of this phase, a ULIRG enters one of two evolutionary paths depending on the dynamics of the merger, the available quantities of gas, and the masses of the black holes in the progenitors. On one branch, the contributions from the starburst and the AGN to the total IR luminosity decline and increase respectively. The IR spectral shapes are heterogeneous, likely due to feedback from AGN-driven winds. Some objects go through a brief QSO phase at the end. On the other branch, the decline of the starburst relative to the AGN is less pronounced, and few or no objects go through a QSO phase. We show that the 11.2 micron PAH feature is a remarkably good diagnostic of evolutionary phase, and identify six ULIRGs that may be archetypes of key stages in this lifecycle.