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Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: arX. iv:1. 002. 3469. v1 [. astr. o-ph. EP]. 18. Feb. 2010. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 19 February 2010 (MN LATEX style file v2.2). Are debris disks self-stirred? G. M. Kennedy and M. C. WyattInstitute of Astronomy, -
MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf8 Jan 2019: MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled using MNRAS LATEX style file v3.0. A gap in HD 92945’s broad planetesimal disc revealed byALMA. S. Marino1,2?, B. Yelverton1, M. Booth3, V. Faramaz4, G. M. Kennedy5,6, L. Matrà7. and M. -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al. -
hd113766_dust_25Sep2007
https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf5 Oct 2007: performed (Watson et al. 2004). The reduction and analysis of the spectra was conducted with. -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group, -
The Astrophysical Journal, 701:2019–2032, 2009 August 20…
https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf1 Aug 2012: 2004). In order to avoid time-consuming peak-up, theobservatory was operated in IRS spectral mapping mode wherea 2 3 raster (spatial dispersion) centered on the star wasperformed (Watson et al.
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