Radio-continuum decrements associated to shadowing from the central warp in transition disc DoAr44

Warps have often been used to explain disc properties, but well characterised examples are important due to their role in disc evolution. Scattered light images of discs with central gaps have revealed sharp warps, such that the outer rings are shadowed by tilted inner discs. The near-IR intensity drops along the ring around TTauri star DoAr44 have been interpreted in terms of a central warp. We report new ALMA observations of DoAr44 in the continuum at 230 GHz and 350 GHz (at ~10 au), along with a new epoch of SPHERE/IRDIS differential polarised imaging taken during excellent weather conditions. The ALMA observations resolve the ring and confirm the decrements proposed from deconvolution of coarse 336 GHz data. The scattered light image constrains the dips, which correspond to a misaligned inner disc with a relative inclination $\xi$ = 21.4 $^{+6.7}_{-8.3}$ deg. The SPHERE intensity profile shows a morphological change compared to a previous epoch that may be interpreted as a variable orientation of the inner disc, from $\xi$ ~30 deg to $\xi$ ~20 deg. The intensity dips probably correspond to temperature decrements, as their mm-spectral index, $\alpha^{230 GHz}_{350 GHz}$ ~2.0 $\pm$ 0.1, is indicative of optically thick emission. The azimuth of the two temperature decrements are leading clockwise relative to the IR-dips, by $\eta$ = 14.95 deg and $\eta$ = 7.92 deg. For a retrograde disc, such shifts are expected from a thermal lag and imply gas surface densities of $\Sigma_g$ = 117 $\pm$ 10 g/cm$^2$ and $\Sigma_g$ = 48 $\pm$ 10 g/cm$^2$. A lopsided disc, with contrast ratio $f_r$=2.4 $\pm$ 0.5, is also consistent with the large continuum crescent.