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7009.pmd
https://people.ast.cam.ac.uk/~wyatt/mwmt08.pdf1 Feb 2008: Because the clearing time of dust in the 24-µm-emitting zone (10–60 AU) is 1–10 m.y. ... HD 69830 is a three-planet systemwith a strong 24-µm excess (see section 4) (Beichman etal., 2005b). -
Dynamics of small bodies in planetary systems Mark C. ...
https://people.ast.cam.ac.uk/~wyatt/wyat08.pdf8 Jul 2008: Rather the dust distribution seen at 24 and 70 µm extendsout to 800 AU [73]. ... Wyatt. Eridani disk which is a narrow ring at 60 AU with a well resolved inner hole[24]. -
arX iv:0 810. 5087 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf3 Nov 2008: Modelling indicates that the extension arises from an edge-on disk of radius0.5 arcsec ( 24 AU). -
Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…
https://people.ast.cam.ac.uk/~wyatt/swd08.pdf29 Apr 2008: 3.1.1. TIMMI2. The observations on TIMMI2 were taken over three runs on 11-12 September 2003, 19-21 November 2003 and 24-26 January2005 (proposals 71.C-0312, ... 123356d G1V O(0.1)e 20.9 14+ 1270 (53) 3 615 (56)128400 G5V 0.3i 20.4 260+ 178 (24) 61+ 64 -
arX iv:0 812. 2475 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/pfwb08.pdf17 Dec 2008: 3.47F(iii) 700 1 No No 24 49 3 0 11 13 0.27 3.97F(iv) 100 1 No No 44 34 1 1 9 11 0.30
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