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MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/kw20.pdf18 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. -
Draft version June 29, 2020Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mdwm20.pdf29 Jun 2020: 1984). It is now. recognised that at least 24% of A-type stars harbour. -
MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mfhk20.pdf30 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 -
MNRAS 000, 1-30 (2020) Preprint 12 October 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/swmn20.pdf15 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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