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Astronomy & Astrophysicsmanuscript no. 8719 c© ESO 2008April 28,…
https://people.ast.cam.ac.uk/~wyatt/swd08.pdf29 Apr 2008: We con-sider a detection to be whereS op > 3. 4.1.1. ... Ndθ = 0.1(dθ/θ)1010(r/θ)R0.5λ Ftot. with Nop andS op determined from equation 1. -
arX iv:0 810. 5087 v1 [ astr o-ph ] ...
https://people.ast.cam.ac.uk/~wyatt/scwm08.pdf3 Nov 2008: arX. iv:0. 810. 5087. v1 [. astr. o-ph. ] 28. Oct. 200. 8Astronomy & Astrophysicsmanuscript no. 10706 c ESO 2008October 28, 2008. Resolved debris disk emission around η Tel: a young Solar Systemor ongoing planet formation? R. Smith1, L.J. Churcher1, -
Dynamics of small bodies in planetary systems Mark C. ...
https://people.ast.cam.ac.uk/~wyatt/wyat08.pdf8 Jul 2008: There are too many uncertaintiesregarding the expected size distribution at very small sizes (e.g., because itdepends on the size distribution created in collisions), and regarding the op-tical properties of
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