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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). 

Tell me why? A case for Human(e) Astrophysics

Artemis, AI, Astronomy, and our place in it. The author asks why do astrophysics at all. To produce results faster, or to turn graduate students into inefficient stand-ins for software? Or because astronomy is one of the most human things we do. It gives us wonder, yes, but also responsibility: to remember the histories of colonialism and militarization tied to our instruments, to use new tools without surrendering judgment, and to insist that people remain the point of the enterprise. The universe is not only something to be computed. It is something to be encountered, interpreted, and loved.

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