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panstarrs.eps
https://people.ast.cam.ac.uk/~wyatt/sjw19.pdf13 Mar 2019: In both Tack. cases, we do not simulate test particles beyond 14 au, but instead. ... the fraction of test particles that are ever members of the Oort cloud. -
A planet-forming circumbinary disc in a polar configura-tion Grant ...
https://people.ast.cam.ac.uk/~wyatt/kmfm19.pdf17 Jan 2019: in Figure 3. To further test this hypothesis, we simulated the response of the disc to perturbations from. ... simulations (see Methods). The main conclusion from the n-body simulations is that test particles. -
A planetesimal orbiting within the debris discaround a white ...
https://people.ast.cam.ac.uk/~wyatt/mgeh19.pdf25 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. -
1911.05131
https://people.ast.cam.ac.uk/~wyatt/tw19.pdf20 Nov 2019: This new survey therefore presents a unique oppor-tunity to test prospective models statistically against a largesample. ... Instead, here we estimate a simple detec-tion threshold to test its significance. -
MNRAS 000, 1–21 (2018) Preprint 11 July 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/yksw19.pdf11 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 -
1906.08797
https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf20 Nov 2019: 4.3. Exploring Hypothetical Exoplanetary SystemArchitecture. Stars that host both a debris disk and one or more exo-planets serve as critical test beds for studying the forma-tion and evolution -
Draft version February 13, 2019Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mwwd19.pdf14 Feb 2019: Nonetheless, we test whether we can. detect a radial dependence of the vertical aspect ratio. ... the two datasets do not allow us to test this hypothe-. -
Draft version April 2, 2019Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/dhcf19.pdf3 Apr 2019: Draft version April 2, 2019Typeset using LATEX twocolumn style in AASTeX62. The Mass of Stirring Bodies in the AU Mic Debris Disk Inferred from Resolved Vertical Structure. Cail Daley,1, 2 A. Meredith Hughes,1 Evan S. Carter,1 Kevin Flaherty,1, 3 -
MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf21 Feb 2019: 5.3.2 Temperature Scenario. To test the possibility of temperature variation as the causeof asymmetry in the outer C18O disc, we measure the av-erage flux in different segments of -
MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf8 Jan 2019: This small difference in χ2 there-fore favours the SR model when compared against the fulleccentric disc model presented in 3 because it has fewerparameters (based on a χ2 difference test
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