Unwinding spiral arms in UG101 and UG103 are driven primarily by tidal interactions and ram pressure stripping respectively, diagnosed from spatially resolved gas/stellar kinematics and stellar population maps.
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With arms wide open: a VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies
Unwinding spiral arms in UG101 and UG103 are driven primarily by tidal interactions and ram pressure stripping respectively, diagnosed from spatially resolved gas/stellar kinematics and stellar population maps.