SMC young stars trace a rotating, highly inclined east-west stretched disk while old stars trace a non-rotating ellipsoid, with a new infalling feature (SEA) appearing in the residuals.
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Unraveling the kinematic and morphological evolution of the Small Magellanic Cloud
SMC young stars trace a rotating, highly inclined east-west stretched disk while old stars trace a non-rotating ellipsoid, with a new infalling feature (SEA) appearing in the residuals.