Galaxy evolution near groups and clusters: ejected satellites and the spatial extent of environmental quenching
Andrew R. Wetzel, Jeremy L. Tinker, Charlie Conroy, Frank C. van den, Bosch

TL;DR
This study investigates how galaxies outside clusters are quenched by environmental effects, highlighting the role of ejected satellites that orbit beyond virial radii and influence galaxy evolution models.
Contribution
It demonstrates that ejected satellite galaxies explain extended environmental quenching beyond virial radii, emphasizing their significant role in galaxy evolution.
Findings
Ejected satellites can orbit beyond the virial radius for several Gyr.
Up to 40% of central galaxies near clusters are ejected satellites.
Ejected satellites experience similar quenching as satellites within halos.
Abstract
Galaxies that are several virial radii beyond groups/clusters show preferentially quiescent star formation rates. Using a galaxy group/cluster catalog from the Sloan Digital Sky Survey, together with a cosmological N-body simulation, we examine the origin of this environmental quenching beyond the virial radius. Accounting for the clustering of groups/clusters, we show that central galaxies show enhanced SFR quenching out to 2.5 virial radii beyond groups/clusters, and we demonstrate that this extended environmental enhancement can be explained simply by 'ejected' satellite galaxies that orbit beyond their host halo's virial radius. We show that ejected satellites typically orbit for several Gyr beyond the virial radius before falling back in, and thus they compose up to 40% of all central galaxies near groups/clusters. We show that a model in which ejected satellites experience the…
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