Answers are grounded in this paper and cite their sources.
Context. Most of the contribution to dust emission in clusters of galaxies comes from late-type galaxies. However, several ejection processes of material from these galaxies could introduce dust in the intracluster media. Even a relatively low abundance of this dust could act as an efficient cooling agent and have a relevant role in the evolution of clusters.
No takes yet. Share an insight, caveat, or question.
Gutiérrez et al. (2014) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: