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  2. MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf
    8 Jan 2019: Middle:Comparison between opposite wedges with a mean PA of 45 (NE,green) and 225 (SW, orange). ... 12 au for the topand bottom panels and 20 au for the middle panel approximately.

  3. Draft version February 13, 2019Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mwwd19.pdf
    14 Feb 2019: 2. The belt spine (Fig. 3, middle) presents little verti-. cal displacement along the midplane and is largely. ... Nonetheless, we test whether we can. detect a radial dependence of the vertical aspect ratio.

  4. A planetesimal orbiting within the debris discaround a white ...

    https://people.ast.cam.ac.uk/~wyatt/mgeh19.pdf
    25 Apr 2019: Manual, http://pencil-code.nordita.org/doc/manual.pdf. 96. C. P. McNally, W. Lyra, J.-C. Passy, A Well-posed Kelvin-Helmholtz Instability Test and. ... S6 &. S7 can be found in the directory pencil-code/samples/2d-tests/WhiteDwarfDisk, using version.

  5. MNRAS 000, 1–21 (2018) Preprint 11 July 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yksw19.pdf
    11 Jul 2019: However, us-ing a Kolmogorov-Smirnov (KS) test, they demonstratedthat the period distributions of their disc-bearing anddisc-free binaries and multiples were not, in fact, differ-ent in a statistically ... Theupper, middle and lower panels show

  6. MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf
    21 Feb 2019: 13CO emission (middle panel) is alsobrighter in the southwest for as far as 2.′′8, beyond whichthe northeast of the disc is brighter. ... 5.3.2 Temperature Scenario. To test the possibility of temperature variation as the causeof asymmetry in the

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