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The debris disc of solar analogue tau Ceti : Herschel observations and dynamical simulations of the proposed multiplanet system

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Figure

Table 1. Herschel observations of τ Ceti.
Figure 1. Cropped Herschel maps of τ Ceti centred on the position of peak 70 µm emission (shown in each panel as a small red circle)
Figure 3. Peak-subtracted images at 70 (left) and 160 µm (right). Here, a PSF has been scaled to the flux of the peak pixel in each band and subtracted fromthe images (see text for details)
Table 3. Observational data from the literature.
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