Galaxy Zoo: major galaxy mergers are not a significant quenching pathway
Anna K. Weigel, Kevin Schawinski, Neven Caplar, Alfredo Carpineti,, Ross E. Hart, Sugata Kaviraj, William C. Keel, Sandor J. Kruk, Chris J., Lintott, Robert C. Nichol, Brooke D. Simmons, Rebecca J. Smethurst

TL;DR
This study investigates the role of major galaxy mergers in quenching star formation and finds they are not a significant pathway for galaxy quenching at low redshift or in recent cosmic history.
Contribution
It provides a comprehensive analysis of stellar mass functions across merger stages, demonstrating that major mergers are unlikely to be the primary quenching mechanism.
Findings
Major mergers are unlikely to be the dominant quenching pathway.
Major merger quenched galaxies constitute only 1-5% of all quenched galaxies at z~0.
Major mergers do not account for the majority of green valley transitions.
Abstract
We use stellar mass functions to study the properties and the significance of quenching through major galaxy mergers. In addition to SDSS DR7 and Galaxy Zoo 1 data, we use samples of visually selected major galaxy mergers and post merger galaxies. We determine the stellar mass functions of the stages that we would expect major merger quenched galaxies to pass through on their way from the blue cloud to the red sequence: 1: major merger, 2: post merger, 3: blue early type, 4: green early type and 5: red early type. Based on the similar mass function shapes we conclude that major mergers are likely to form an evolutionary sequence from star formation to quiescence via quenching. Relative to all blue galaxies, the major merger fraction increases as a function of stellar mass. Major merger quenching is inconsistent with the mass and environment quenching model. At z~0 major merger quenched…
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