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L and N in the UK
https://people.ast.cam.ac.uk/~vasily/oxford_homepage/ln.html13 Jul 2010: The amount of duty being evaded on these sales was well in excess of 200,000. -
arX iv:1 009. 0248 v1 [ astr o-ph .SR ...
https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf2 Sep 2010: 0.5. 1-50. 51-100. 101-150. 151-200. 201-250. 251-300. 301-350. 351-400. 401-450. 451-500. -
Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…
https://people.ast.cam.ac.uk/~wyatt/kw11.pdf25 Nov 2010: C. Wyatt. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400of. fset. (Sa. turn. rad. ii). -100 -50 0 50 100offset (arcmin). -
arX iv:1 001. 5177 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/gw10.pdf29 Jan 2010: 200 mJy (Wyatt 2005) and the corresponding limit for ISOwas around 90 mJy (Decin et al. -
Are Debris Disks Self-Stirred?
https://people.ast.cam.ac.uk/~wyatt/kw10.pdf19 Feb 2010: Our model shows a fairly slow decline untilafter 200–600 Myr, when stirring reaches the outer diskedge and the excess decreases more rapidly because massis being lost at all radii. ... Given that PRdrag is unlikely to be the cause, the further drop in -
arX iv:1 004. 0644 v1 [ astr o-ph .EP ...
https://people.ast.cam.ac.uk/~wyatt/sw10.pdf6 Apr 2010: arX. iv:1. 004. 0644. v1 [. astr. o-ph. EP. ] 5. Apr. 201. 0Astronomy & Astrophysicsmanuscript no. astars˙3rd c ESO 2010April 6, 2010. Warm dusty discs: Exploring the A star 24µm debris populationR. Smith1,2 and M.C. Wyatt2. 1 Astrophysics Group,
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