Detecting cold gas in a hot supercluster

Detecting cold gas in a hot supercluster

The Shapley Supercluster is widely recognised as the most massive gravitationally bound structure in the local universe.The supercluster is made up of 11 galaxy clusters and groups and extends across ~ 260 megaparsecs. At its⁡ core, which this paper focuses on, are five clusters. This core hosts several radio haloes,which are caused by shock-heated gas from the Intracluster medium (ICM) and is evidence of ongoing cluster merger activity. This supercluster core is highly dynamically active (full of cluster-cluster mergers), which could influence the evolution of galaxies within the core. This paper examines the evolution of galaxies by observing the cold gas within galaxies (i.e. the neutral hydrogen) and compares several galaxy properties to do so (see also: this previous Astrobite featuring ram-pressure stripped galaxies in the Shapley Supercluster). 

Guest: The closest look into the largest nearby cosmic structures: a foray into the Fornax galaxy cluster

Guest: The closest look into the largest nearby cosmic structures: a foray into the Fornax galaxy cluster

Galaxy clusters are collections of galaxies that are bound together by gravity. They are the largest structures that exist in our Universe, and their mass is dominated by the hot gas that lies between galaxies called the intracluster medium. One of the closest galaxy clusters is Fornax, and it was recently studied in detail using the MeerKAT radio telescope in South Africa. This bite dives deep into a study of the magnetic field of this cluster and the implications the results have of our understanding of clusters of galaxies.