The insignificance of major mergers in driving star formation at z~2

TL;DR

This study shows that major mergers contribute minimally to star formation at z~2, with other processes like cold accretion playing a more significant role in galaxy growth during this epoch.

Contribution

It provides a quantitative analysis of the limited role of major mergers in star formation at z~2, challenging their perceived dominance in galaxy evolution.

Findings

Major mergers account for approximately 15% of star formation at z~2.

Non-interacting late-type galaxies host the majority of star formation.

Star formation enhancement in mergers is modest, with a ratio of about 2.2:1 compared to non-interacting galaxies.

Abstract

We study the significance of major-merger-driven star formation in the early Universe, by quantifying the contribution of this process to the total star formation budget in 80 massive (M* > 10^10 MSun) galaxies at z~2. Employing visually-classified morphologies from rest-frame V-band HST imaging, we find that 55+/-14% of the star formation budget is hosted by non-interacting late-types, with 27+/-8% in major mergers and 18+/-6% in spheroids. Given that a system undergoing a major merger continues to experience star formation driven by other processes at this epoch (e.g. cold accretion, minor mergers), ~27% is an upper limit to the major-merger contribution to star formation activity at this epoch. The ratio of the average specific star formation rate in major mergers to that in the non-interacting late-types is ~2.2:1, suggesting that the enhancement of star formation due to major merging is typically modest, and that just under half the star formation in systems experiencing major mergers is unrelated to the merger itself. Taking this into account, we estimate that the actual major-merger contribution to the star formation budget may be as low as ~15%. While our study does not preclude a major-merger-dominated era in the very early Universe, if the major-merger contribution to star formation does not evolve strongly into larger look-back times, then this process has a relatively insignificant role in driving stellar mass assembly over cosmic time.