  Observations of an unprecedented quality made by ALMA on the Red Rectangle of
CO(3-2) and CO(6-5) emissions are analysed jointly with the aim of obtaining as
simple as possible a description of the gas morphology and kinematics. Evidence
is found for polar conical outflows and for a broad equatorial torus in
rotation and expansion. Simple models of both are proposed. Comparing CO(6-5)
and CO(3-2) emissions provides evidence for a strong temperature enhancement
over the polar outflows. Continuum emission (dust) is seen to be enhanced in
the equatorial region. Observed asymmetries are briefly discussed.
