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842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 Sep 2007: assumingF /F p 0.1disk a limit of , based on Su et al. ... 3. Stellar multiplicity.—With 50% of target stars havinganother star as a companion. -
Observing Kepler stars with WISE
https://people.ast.cam.ac.uk/~wyatt/kw12.pdf7 Jul 2012: Previous effortsfor theHerschel (Pilbratt et al. 2010) Disc Emission via a Bias-free. ... A total of 144655sources have a WISE detection in at least one band. -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: Weshow that there is no significant statistical difference between fractional excessesof A-stars. ... 5). We also assume that the central star acts like a black-body. -
arX iv:1 312. 4531 v2 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kmlm13.pdf21 Jan 2014: a useful evolutionary sequence it is important to interpret in-dividual objects carefully. ... 4.8. Schneider et al. (2013)report a detection in the XMM-Newton Serendipitous Source Cat-alog (Watson et al. -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: possibilitiesinclude dynamical scattering by a migrating planet, see e.g.Gomes et al. ... This source together with HD 31295 andHD 38206 are described in Appendix A. -
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...
https://people.ast.cam.ac.uk/~wyatt/wbpc09.pdf25 Oct 2009: by postulating a populationof parent planetesimals on highly eccentric orbits (e 0.3). ... Rcc(Dmax) = KMtotv8/3k (a)a. 3(4πImax)1S(e), (16). S2d(e) =X. r̄. r̄2dr̄1σ̄(r̄)2〈[vrel/vk(a)]8/3〉(r̄), (17). -
Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...
https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf5 Jul 2011: Four 3’ scan legs wereperformed per map with a 2” separation between legs. ... 2008) and to a theoretical PSF (gen-. 2010 RAS, MNRAS 000, 1–20. -
hd113766_dust_25Sep2007
https://people.ast.cam.ac.uk/~wyatt/lcwm08.pdf5 Oct 2007: within a massive comet or asteroid (processed, differentiated planetesimals) belt, (iv) recent col-. ... performed (Watson et al. 2004). The reduction and analysis of the spectra was conducted with. -
Publications of the Astronomical Society of Australia (PASA)doi:…
https://people.ast.cam.ac.uk/~wyatt/khna21.pdf23 Nov 2021: These instru-ments reveal a wealth of substructures within disks, forboth targeted (e.g. ... We assumehere a gas-to-dust mass ratio of 100 and indicate the. -
MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/kw20.pdf18 Aug 2020: We start with a simple estimate. Assuming the PPDmass to be 0.1M? ... A-stars with2 solar masses) can be higher by a factor 2.7.
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