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  2. MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/kw20.pdf
    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.
  3. Draft version June 29, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mdwm20.pdf
    29 Jun 2020: 1984). It is now. recognised that at least 24% of A-type stars harbour.
  4. MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mfhk20.pdf
    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
  5. MNRAS 000, 1-30 (2020) Preprint 12 October 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/swmn20.pdf
    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.

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