JWST observations reveal extended [Ne VI] emission in the Phoenix cluster, tracing a recent burst of cooling at 10^5.5 K with an inferred rate of 5,000-23,000 solar masses per year.
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Directly Imaging the Cooling Flow in the Phoenix Cluster
JWST observations reveal extended [Ne VI] emission in the Phoenix cluster, tracing a recent burst of cooling at 10^5.5 K with an inferred rate of 5,000-23,000 solar masses per year.