Science & ResearchSep 4, 2026
Rapid quenching and early gas depletion in the core of a galaxy protocluster at z=2.2
Understanding how galaxy evolution is affected in forming high-z overdensities is a major open question in modern astrophysics.
Understanding how galaxy evolution is affected in forming high-z overdensities is a major open question in modern astrophysics. Here, we present the average properties of the quiescent galaxy population recently identified in the core of the Spiderweb protocluster at z = 2.16.…
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