Quantifying the role of ram pressure stripping of galaxies within galaxy groups
Tutku Kolcu, Jacob P. Crossett, Callum Bellhouse, Sean McGee

TL;DR
This study challenges the belief that ram pressure stripping is rare in galaxy groups by identifying 45 candidates, suggesting it could be a key mechanism for galaxy quenching in such environments.
Contribution
It provides observational evidence and a physical model showing ram pressure stripping occurs in galaxy groups, not just clusters, and may be a dominant quenching process.
Findings
45 ram-pressure stripped galaxy candidates identified
Candidates are mostly blue, star-forming, first infallers
Ram pressure stripping is plausible at group halo masses
Abstract
It is often stated that the removal of gas by ram pressure stripping of a galaxy disk is not a common process in galaxy groups. In this study, with the aid of an observational classification of galaxies and a simple physical model, we show that this may not be true. We examined and identified 45 ram-pressure stripped galaxy candidates from a sample of 1311 galaxy group members within 125 spectroscopically-selected galaxy groups. 13 of these galaxies are the most secure candidates with multiple distinct features. These candidate ram pressure stripped galaxies have similar properties to those found in clusters -- they occur at a range of stellar masses, are largely blue and star-forming and have phase-space distributions consistent with being first infallers into their groups. The only stand-out feature of these candidates is they exist not in clusters, but in groups, with a median halo…
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