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MNRAS 000, 1–16 (2017) Preprint January 22, 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/rwmk18.pdf22 Jan 2018: 2016). As such, HR8799 isan ideal test system for planet formation and evolution the-ories, as interactions between planets themselves and withdebris can be investigated. ... simulations from the four known planets interacting with a pop-ulation of test -
arX iv:1 803. 1126 5v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/edhm18.pdf2 Apr 2018: ture work. In contrast, it is important for the present. work to treat all systems in a uniform way.For detected excesses, we test whether our SZ model is. -
The HOSTS Survey for Exozodiacal Dust: Preliminaryresults and future…
https://people.ast.cam.ac.uk/~wyatt/ekdh18.pdf30 Jul 2018: 4. The resultsof Fisher’s exact test to check if differences in the detection rates are significant are shown in Table 3. -
Mon. Not. R. Astron. Soc. 000, 1–23 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kmwk18.pdf22 Nov 2018: which we will test further by comparing to models inthe next subsection 4.2. -
MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf31 Jul 2018: MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled using MNRAS LATEX style file v3.0. A gap in the planetesimal disc around HD 107146 andasymmetric warm dust emission revealed by ALMA. S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S. -
MNRAS 479, 2649–2672 (2018) doi:10.1093/mnras/sty1677Advance Access…
https://people.ast.cam.ac.uk/~wyatt/kwtm18.pdf30 Jul 2018: We start each simulation with 2000 test particles that all have asimilar pericentre and apocentre {q, Q} spread in a narrow rangedefined by a grid (see Fig. ... We ran N-body simulations to follow the evolution of test particlesinitially randomly located -
MNRAS 000, 1–13 (2018) Preprint 23 August 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/irgm18.pdf23 Aug 2018: In order to test the viability of this scenario, we followRappaport et al. -
Debris Disks: Probing Planet Formation Mark C. Wyatt Abstract ...
https://people.ast.cam.ac.uk/~wyatt/wyat18.pdf20 Jul 2018: 2017). Giant impacts at 10s of au. Disk structure provides an alternative test for the possible growth of dwarf planetswithin debris disks. -
Draft version January 1, 2018Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/mwoa18.pdf2 Jan 2018: Two. of the spectral windows were set in frequency division. mode and allowed us to test for the presence of spec-. -
MNRAS 000, 1–11 (2018) Preprint 27 June 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/sbbc18.pdf31 Jul 2018: For another test, we have examined our timeseries photometry for variations even down to 40-second induration, but we find no significant dips or flares on any fasttime scales.
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