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MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...
https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf3 Jul 2007: SCUBA camera on the James Clerk Maxwell Telescope. -
SUBMILLIMETER IMAGES OF A DUSTY KUIPER BELT AROUND � ...
https://people.ast.cam.ac.uk/~wyatt/wgdc05.pdf19 Apr 2006: 2. OBSERVATIONS. 2.1. Submillimeter. The submillimeter observations of Corvi were made usingthe Submillimeter Common-User Bolometer Array (SCUBA)at the James Clerk Maxwell Telescope (JCMT). -
STARS draft version, October 28, 2012 2 Contents 1 ...
https://people.ast.cam.ac.uk/~stars/doc/stars.pdf14 Mar 2013: It is based on A Simple Makefile Tutorial 1, whichWarrick Ball found on the website of Bruce Maxwell. ... 1http://www.cs.colby.edu/maxwell/courses/tutorials/maketutor/. 9. OPACITY OUT OF RANGE TF FR FKL FKH. followed by four numbers. -
2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…
https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf22 Mar 2024: Leisenring,19. Maxwell A. Millar-Blanchaer,20 Laurent Pueyo,7 Shrishmoy Ray ,17 Steph Sallum,21 Karl R. -
MNRAS 435, 1037–1046 (2013) doi:10.1093/mnras/stt1293Advance Access…
https://people.ast.cam.ac.uk/~wyatt/phwk13.pdf12 Nov 2013: In the frame-work of the ongoing SCUBA-2 Observations of Nearby Stars, the instrument SCUBA-2 on theJames Clerk Maxwell Telescope was used to provide measurements of 450 and 850 -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06.pdf17 Oct 2022: and the most probablespeed is v =. 2kT/m for a Maxwell-Botzmann distribution. In cooler stars, where pressure broadening is most important, collisionswith neutral hydrogen atoms are the main source of -
arX iv:1 008. 0865 v2 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/cws10.pdf22 Aug 2010: 1999) using Maxwell-Garnett effective mediumtheory. The optical properties of the grains were calculated usingMie theory, Rayleigh-Gans theory and Geometric Optics in the ap-propriate size regimes (Bohren & Huffman 1983). -
arX iv:0 810. 5087 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf3 Nov 2008: 1999).Dielectric constants were calculated using Maxwell-Garnett ef-fective medium theory and optical properties calculated usingMie theory, Rayleigh-Gans theory and Geometric Optics in theappropriate size regimes (Bohren & Huffman 1983). -
Draft version May 29, 2015Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/cwmm15.pdf14 Sep 2015: 103 M in silicate grains mixed withices (using the Maxwell-Garnett rule). -
cv.dvi
https://people.ast.cam.ac.uk/~gpe/cv.pdf24 Jan 2012: College, Cambridge.1984 Senior Research Fellowship King’s College, Cambridge.1990 Maxwell Medal & Prize Institute of Physics.1990 Vainu Bappu Prize Astronomical Society of India.1991 Fairchild Distinguished Scholar California Institute -
Draft version December 10, 2012Preprint typeset using LATEX style ...
https://people.ast.cam.ac.uk/~wyatt/bmkb12.pdf10 Dec 2012: 2005; Beichman et al. 2006; Brydenet al. 2009), the James Clerk Maxwell Telescope (Hollandet al. -
arX iv:a stro -ph/ 0504 086 v1 4 A ...
https://people.ast.cam.ac.uk/~wyatt/srms05.pdf19 Apr 2006: The 850 µm map of Vega obtained by Holland et al.(1998) with the Submillimeter Common-User Bolome-ter Array (SCUBA) on the James Clerk Maxwell Tele-scope shows an extended, -
The clumpy structure of epsilon Eridani's debris disc revisited…
https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf27 Mar 2023: ar 2. 023. 2 M. Booth et al. Bolometer Array (SCUBA) image of the disc taken at theJames Clerk Maxwell Telescope (JCMT) (Greaves et al.1998), there have been claims of -
Mon. Not. R. Astron. Soc. 334, 589–607 (2002) Collisional ...
https://people.ast.cam.ac.uk/~wyatt/wd02.pdf19 Apr 2006: 1.Recently the structure of the disc was mapped at both 450 and850 µm using SCUBA at the James Clerk Maxwell Telescope(JCMT) (Holland et al. ... We usethe optical constants for each of the components taken from Li &Greenberg (1997, 1998) and compute -
Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf5 May 2017: 1991). With the introduc-tion of the Submillimetre Common-User Bolometer Array(SCUBA) to the James Clerk Maxwell Telescope (JCMT),Greaves et al. -
MNRAS 000, 1–14 (0000) Preprint 28 April 2017 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/mwkh17.pdf5 May 2017: 2 (SCUBA2) installedin the James Clerk Maxwell Telescope (JCMT), thus, incorporatinginformation from small and large angular scale structure. -
58419 1321..1340
https://people.ast.cam.ac.uk/~wyatt/wyat03b.pdf19 Apr 2006: RESONANT TRAPPING OF PLANETESIMALS BY PLANET MIGRATION: DEBRIS DISK CLUMPSAND VEGA’S SIMILARITY TO THE SOLAR SYSTEM. M. C. WyattUK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, UK; wyatt@roe.ac.uk. Received 2003 June 11; -
DRAFT VERSION MAY 24, 2022Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/hcrs22.pdf24 May 2022: Sasha Hinkley ,1 Aarynn L. Carter ,2 Shrishmoy Ray ,1 Andrew Skemer,2 Beth Biller,3 Elodie Choquet,4 Maxwell A. -
Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed ...
https://people.ast.cam.ac.uk/~wyatt/cwds11.pdf5 Jul 2011: 1999) using Maxwell-Garnetteffective medium theory. The optical properties of the grains werecalculated using Mie theory, Rayleigh-Gans theory and GeometricOptics in the appropriate size regimes (Bohren & Huffman 1983).This composition -
/astro/p7scch2/AUMic/paper/figures/all.eps
https://people.ast.cam.ac.uk/~wyatt/wlke15.pdf16 Jun 2015: Recently,a dust halo was also detected in far-IR resolvedHerschelandJCMT (James Clerk Maxwell Telescope) images by Matthews etal.
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