Studying the kinematic asymmetries of disks and post-coalescence mergers using a new `kinemetry' criterion

Details Studying the kinematic asymmetries of disks and post-coalescence mergers using a new `kinemetry' criterion Studying the kinematic asymmetries of disks and post-coalescence mergers using a new `kinemetry' criterion

2012-03-08

arxiv.org/abs/1203.1930v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

15 figures, 19 pages

Scientific paper

We have obtained VIMOS/VLT optical integral field spectroscopy (IFS) data for a sample of 4 LIRGs which have been selected at a similar distance ($\sim$ 70 Mpc) to avoid relative resolution effects. They have been classified in two groups (isolated disk and post-coalescence mergers) according to their morphology. The $kinemetry$ method (developed by Krajnovic and coworkers) is used to characterize the kinematic properties of these galaxies and to discuss new criteria for distinguishing their status. We present and discuss new kinematic maps (i.e., velocity field and velocity dispersion) for these four galaxies. The morphological and kinematic classifications of these systems are consistent, with disks having lower kinematic asymmetries than post-coalescence mergers. We then propose and discuss a new kinematic criterion to differentiate these two groups. This criterion distinguishes better these two categories and has the advantage of being less sensitive to angular resolution effects. According to the previous criteria,the present post-coalescence systems would have been classified as disks. This indicates that the separation of disks from mergers is subjective to the definition of `merger'. It also suggests that previous estimates of the merger/disk ratio could have been underestimated, but larger samples are necessary to establish a firmer conclusion.

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