Facial reconstruction

Search LJMU Research Online

Browse Repository | Browse E-Theses

Galaxy and Mass Assembly (GAMA): merging galaxies and their properties

De Propris, R, Baldry, IK, Bland-Hawthorn, J, Brough, S, Driver, SP, Hopkins, AM, Kelvin, L, Loveday, J, Phillipps, S and Robotham, ASG (2014) Galaxy and Mass Assembly (GAMA): merging galaxies and their properties. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 444 (3). pp. 2200-2211. ISSN 0035-8711

This is the latest version of this item.

1407.4996v1.pdf - Accepted Version

Download (1MB) | Preview


We derive the close pair fractions and volume merger rates for galaxies in the Galaxy and Mass Assembly (GAMA) survey with −23 < Mr < −17 (ΩM = 0.27, ΩΛ = 0.73, H0 = 100 km s−1 Mpc−1) at 0.01 < z < 0.22 (look-back time of <2 Gyr). The merger fraction is approximately 1.5 per cent Gyr−1 at all luminosities (assuming 50 per cent of pairs merge) and the volume merger rate is ≈3.5 × 10−4 Mpc−3 Gyr−1. We examine how the merger rate varies by luminosity and morphology. Dry mergers (between red/spheroidal galaxies) are found to be uncommon and to decrease with decreasing luminosity. Fainter mergers are wet, between blue/discy galaxies. Damp mergers (one of each type) follow the average of dry and wet mergers. In the brighter luminosity bin (−23 < Mr < −20), the merger rate evolution is flat, irrespective of colour or morphology, out to z ∼ 0.2. The makeup of the merging population does not appear to change over this redshift range. Galaxy growth by major mergers appears comparatively unimportant and dry mergers are unlikely to be significant in the buildup of the red sequence over the past 2 Gyr. We compare the colour, morphology, environmental density and degree of activity (BPT class, Baldwin, Phillips & Terlevich) of galaxies in pairs to those of more isolated objects in the same volume. Galaxies in close pairs tend to be both redder and slightly more spheroid dominated than the comparison sample. We suggest that this may be due to ‘harassment’ in multiple previous passes prior to the current close interaction. Galaxy pairs do not appear to prefer significantly denser environments. There is no evidence of an enhancement in the AGN fraction in pairs, compared to other galaxies in the same volume.

Item Type: Article
Additional Information: This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record "Galaxy and Mass Assembly (GAMA): merging galaxies and their properties", MNRAS 444(3), pp.2200-2211 is available online at: http://dx.doi.org/10.1093/mnras/stu1452
Uncontrolled Keywords: 0201 Astronomical And Space Sciences
Subjects: Q Science > QB Astronomy
Divisions: Astrophysics Research Institute
Related URLs:
Date Deposited: 27 Oct 2015 08:53
Last Modified: 04 Sep 2021 14:02
DOI or ID number: 10.1093/mnras/stu1452
URI: https://researchonline.ljmu.ac.uk/id/eprint/1877

Available Versions of this Item

View Item View Item