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SpaceMost baryons in present-day galaxy clusters exist as hot gas (≳107 K), forming the intracluster medium (ICM)1. Cosmological simulations predict that the mass and temperature of the ICM decline towards earlier times, as intracluster gas in younger clusters is still assembling and being heated2–4. To date, hot ICM has been securely detected only in a few systems at or above z ≈ 2, leaving the timing and mechanism of ICM assembly uncertain5–7. Here…See the Story
Sunyaev–Zeldovich detection of hot intracluster gas at redshift 4.3
75% Center coverage: 8 sources
