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We consider the response of a protostellar disc to a tidally induced warp and the resultant changes in the spectral energy distribution (SED). We argue that for typical protostellar disc parameters the warp is communicated through the disc in a wave‐like fashion. We find that the main effects of the warp tend to be at large radii (  R ≳ 30  au) and, for sufficiently small viscosity, can be quite long‐lived. This can result in non‐uniform illumination of the disc at these radii and can induce significant changes to the SED at wavelengths  λ≳ 100 μm .

The observable effects of tidally induced warps in protostellar discs