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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. -
Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…
https://people.ast.cam.ac.uk/~wyatt/swd08.pdf29 Apr 2008: 2005), thoughtto be there because this is a young (12Myr, Zuckerman et al. ... We con-sider a detection to be whereS op > 3. 4.1.1. -
MNRAS 000, 1–27 (2020) Preprint 27October 2020 Compiled…
https://people.ast.cam.ac.uk/~wyatt/lwak20.pdf10 Feb 2021: 2017), a possibility also not ruled out by far-IRsurveys of star forming regions. ... Withinthe inner 0.68′′ radius circle there is a 2.8𝜎 significant detection. -
arX iv:1 310. 6936 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/gkte13.pdf28 Oct 2013: Kervella P., Thévenin F., Di Folco E., Ségransan D., 2004,A&A 426, 297. ... von Braun K. et al., 2011, ApJ 729, L26. Watson C.A. -
Five steps in the evolution from protoplanetary to debrisdisk ...
https://people.ast.cam.ac.uk/~wyatt/wpkm15.pdf17 Dec 2014: mass component of a protoplanetary disk, is no longer. present in debris disks. ... this denomination. A catalogue summarising this class. is given in Thé et al. -
MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/cmfk19.pdf11 Apr 2019: A typical valuefor λmax within our galaxy is 550 nm (Serkowski et al. ... 2010). is the Sun at its centre, a fact which naturally explains thephenomenon. -
arX iv:1 408. 4116 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/kw14.pdf22 Aug 2014: Infra-red excess detections are generally well approxi-mated by a single blackbody. ... For example,ζ Lep shows evidence for extra emissionabove a blackbody around 10µm (Fig. -
arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf29 Apr 2016: arX. iv:1. 604. 0828. 6v1. [ast. ro-p. h.E. P]. 28 A. ... by high orbital eccentricity comets,is likewise difficult to achieve from a dynamical perspective. -
Accepted to ApJ: October 28, 2015Preprint typeset using LATEX ...
https://people.ast.cam.ac.uk/~wyatt/agrj15.pdf2 Nov 2015: M. Ansdell1,10, E. Gaidos2,3,4,10, S. A. Rappaport5, T. L. Jacobs6, D. ... M. LaCourse6, K. J. Jek6, A. W. Mann7,10, M.C. Wyatt8, G. -
, DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...
https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf23 Dec 2017: WATSON,130 R.C. WEIR,4. KLAUS WENZEL,131 MICHAEL W. WILLIAMSON,56 JASON T. WRIGHT,10, 11, 132 M. ... TheLCOGT observations are a product of a successful crowd-funding effort through Kickstarter3. -
arX iv:1 311. 2977 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/mksb13.pdf14 Nov 2013: How-ever, given that all three lie along a line of Fν λ. ... 2009).The suggestion that the entire HR 8799 system may be. coplanar is consistent with the results of Watson et al.(2011) and Greaves et al. -
MNRAS 000, 1–19 (2015) Preprint 4 July 2018 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mcwb18.pdf31 Jul 2018: This implies a very massive initial disc and efficientplanetesimal formation at large radii. ... parameters toour reference parametric model (3-power law surface densitywith a Gaussian gap). -
TLA_large
https://people.ast.cam.ac.uk/~wyatt/tgmk14.pdf4 Dec 2014: Key words: surveys – binaries: general – circumstellar matter – stars: individual: A-stars –infrared: stars. ... Mi. HD. 8769. 6A. 7V28. 24. 450. UM. a(3. ,4). 22.0. -
arX iv:1 403. 6186 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/mmek14.pdf2 Jul 2014: J.P. Marshall, A. Moro-Martı́n, et al.: Herschel observations of exoplanet host stars. ... plored for a broad range of ages by e.g. Decin et al. -
Space Science Reviews manuscript No.(will be inserted by the ...
https://people.ast.cam.ac.uk/~wyatt/wj16.pdf15 Mar 2016: 2007), but could have a dramatic effect on the emission spectrum of theplanet. ... Typically the total mass of debris created in a giant impact iswell known. -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: The origin of this hot dust is a matter of consid-erable debate. ... Nevertheless,a growing number of systems host planets and debris(Wyatt et al. -
Observations, Modeling and Theory of Debris Disks Brenda C. ...
https://people.ast.cam.ac.uk/~wyatt/mkwb14.pdf7 Jan 2014: stars are statistically indistinguishable,a result supported by DUNES data (Eiroa et al. ... Even in a transport-dominated disk, the largest planetes-imals are dominated by collisions.
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