Evidence for anisotropic quenching in massive galaxy clusters at $z\approx 0.5$

Abstract

A recent observational result finds that the quenching of satellites in groups at $z=0.08$ has an angular dependence relative to the semi-major axis of the central galaxy. This observation is described as `anisotropic quenching' or `angular conformity'. In this paper I study the variation in the colour of a mass limited sample of satellite galaxies relative to their angle from the major axis of the Brightest Cluster Galaxy in the CLASH clusters up to $z\sim 0.5$, 4 Gyr further in lookback time. The same result is found: galaxies close to the major axis are more quenched than those along the minor axis. I also find that the star-forming galaxies tend to avoid a region +/-45 degrees from the major axis. This quenching signal is thought to be driven by AGN outflows along the minor axis, reducing the density of the intergalactic medium and thus the strength of ram pressure. Here I will discuss potential alternative mechanisms. Finally, I note that the advent of the Legacy Survey of Space and Time (LSST) and Euclid surveys will allow for a more detailed study of this phenomenon and its evolution.

This has been edited by the author to match the accepted version

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Cited by in corpus (6)

• A jolt to the system: ram pressure on low-mass galaxies in simulations of the Local Group
• Evolution of central galaxy alignments in simulations
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• Anisotropic correlation functions as tracers of central galaxy alignments in simulations
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• Alignment of the central galaxies with the environment