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arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bw10.pdf27 Jul 2010: The outcome is summarisedin Fig. 6. 4.4.1 Radiation pressure. Radiation pressure is a radial force which acts in the op-posite direction to the star’s gravity. -
Mon. Not. R. Astron. Soc. 000, 1–21 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kmkm20.pdf8 Jul 2020: Finally, the detection of this gas is also a new op-portunity to study mechanisms that can transport angularmomentum in discs and may be beneficial for our under-standing of the ... We also compute CN masses in non-LTE assuming op-tically thin emission -
MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/aght19.pdf17 Jan 2020: Evidence of misaligned inner discs has also beenrecently inferred for several systems using high-contrast op-tical/infrared images, which have revealed shadows in theouter disc cast by unseen inclined inner -
MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf23 Sep 2016: before through modelling observations of op-tical and near-IR scattered light from the dust disk (e.g.Ahmic et al. -
Draft version May 29, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf14 Sep 2015: map reproduces the input op-tical depths very closely. -
arX iv:0 810. 5087 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf3 Nov 2008: arX. iv:0. 810. 5087. v1 [. astr. o-ph. ] 28. Oct. 200. 8Astronomy & Astrophysicsmanuscript no. 10706 c ESO 2008October 28, 2008. Resolved debris disk emission around η Tel: a young Solar Systemor ongoing planet formation? R. Smith1, L.J. Churcher1, -
MNRAS 000, 1–13 (2018) Preprint 23 August 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/irgm18.pdf23 Aug 2018: 2017, Fig. A1, bottom). The high op-tical depth in the mid-plane would in fact shield the smallgrains from sublimation. -
arX iv:s ubm it/03 5390 2 [ astr o-ph ...
https://people.ast.cam.ac.uk/~wyatt/bw11.pdf8 Nov 2011: It is interesting to note that the op-timum position for the inner planet is not as close to thestar as the outer planet could possibly scatter particles -
arX iv:a stro -ph/ 0504 086 v1 4 A ...
https://people.ast.cam.ac.uk/~wyatt/srms05.pdf19 Apr 2006: To probe the nature of the Vega disk further, wehave fitted it with models including realistic grain op-tical properties. -
Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...
https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf2 Nov 2015: Road, Cambridge, UK9 Department of Astronomy, Yale University, New Haven, CT10 Visiting Astronomer, NASA Infrared Telescope Facility, op-.
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