3D spectroscopy with VLT/GIRAFFE - II: Are Luminous Compact Galaxies merger remnants ?

TL;DR

This study uses 3D spectroscopy to analyze the kinematics of luminous compact galaxies at intermediate redshifts, revealing that most exhibit complex motions indicative of merger activity, supporting the spiral rebuilding scenario.

Contribution

First detailed 3D velocity field analysis of Luminous Compact Galaxies at z=0.4-0.75, providing evidence for their merger-driven evolution.

Findings

Only 18% show typical rotating disk kinematics.

About half are non-relaxed or merger remnants.

Supports the spiral rebuilding scenario for galaxy evolution.

Abstract

Luminous Compact Galaxies are enigmatic sources by many aspects. They can reach the luminosity of the Milky Way within a radius of only a few kpc. They also represent one of the most rapidly evolving populations of galaxies since they represent up to 1/5 of the luminous galaxies at redshift z= 0.7 while being almost absent in the local Universe. The measurement of their dynamics is crucial to our understanding of LCGs since this has the potential of telling us which physical process(es) that drives them, and ultimately to link them to the existing present-day galaxies. Here we derive the 3 dimensional velocity fields and velocity dispersion (sigma) maps of 17 Luminous Compact Galaxies selected from the Canada France Redshift Survey and the Hubble Deep Field South with redshifts ranging from z=0.4 to z=0.75. We find that only 18% of them show rotational velocity fields typical of rotating disks, the others showing more complex kinematics. Assuming that LCGs are not too far from equilibrium, about half of LCGs then appear to be either non-relaxed objects, or objects that are not supported by velocity dispersion alone. This supports the view that an important fraction of LCGs are probably mergers. It brings additional support to the ``spiral rebuilding scenario'' in which LCGs correspond to a previous or post-merger phase before the disk re-building.