Fig. 1

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12CO zeroth moment images of the discs around multiple stars in the Taurus star-forming region observed in the new ALMA observations. All bars in the bottom right of each panel are of 1″ in length, which is ~140 au at the typical distance of the Taurus region. The FWHM beam size is shown in the bottom left of each panel. In each image, the colour scale has the peak flux as the maximum, and two times the image rms as minimum. White contours show five times the rms of the continuum emission. The components of the systems are labelled. The label for any undetected secondary components in the continuum emission is not shown.
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