JWST and ALMA data provide the earliest direct evidence of ram-pressure stripping in a post-starburst galaxy at z=3.06, implying the process can quench star formation in nascent groups at z>3.
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ALMA observations of five DSFGs in the Spiderweb protocluster reveal disturbed molecular gas kinematics, field-like gas fractions that are lower in massive/AGN hosts, and declining gas content and sSFR with proximity to the central galaxy.
citing papers explorer
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A Post-starburst Galaxy Undergoing Ram-pressure Stripping at Redshift 3.06
JWST and ALMA data provide the earliest direct evidence of ram-pressure stripping in a post-starburst galaxy at z=3.06, implying the process can quench star formation in nascent groups at z>3.
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Chaotic Molecular Gas in Five Dusty Star-forming Galaxies in the Spiderweb Protocluster at $z = 2.16$
ALMA observations of five DSFGs in the Spiderweb protocluster reveal disturbed molecular gas kinematics, field-like gas fractions that are lower in massive/AGN hosts, and declining gas content and sSFR with proximity to the central galaxy.