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18 Aug 2020: 8.1 1.6 23 100.0 100.0 24.3 2.1e-03 7.9e-02 1.2e03 4.1e03 0.3 5.5. ... 24). purposes, as we only wish to demonstrate that the Kuiperbelt is not affected by the mass problem.

29 Jun 2020: 1984). It is now. recognised that at least 24% of A-type stars harbour.

30 Jan 2020: 2007b) to fit the infrared excess evolution at 24 and70 µm in nearby A stars (Rieke et al. ... Wyatt et al. used the distri-bution of observed 24 and 70 µm excess as a function ofage to constrain the initial distribution of disc radii (ap-proximating

15 Oct 2020: vimppξq “b. v2esc. ξvpl˘2. (24). These test impactor properties, labelled by the outcome they haveon the atmosphere, are shown in Table 1.