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  2. arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...

    https://people.ast.cam.ac.uk/~wyatt/bw10.pdf
    27 Jul 2010: Parameter Orginal value New value. Mmid 10.0 7.8 MDc 60.0 1.9kme 0.05 0.05. ... lation that incorporates the optical properties of realisticgrains, to find new values for this parameter set.

  3. arX iv:1 004. 0644 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/sw10.pdf
    6 Apr 2010: Su et al. (2006) presented new 24 and 70µmphotometry which also confirms the excess.

  4. arX iv:1 012. 3079 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/mw11.pdf
    15 Dec 2010: arX. iv:1. 012. 3079. v1 [. astr. o-ph. EP. ] 14. Dec. 201. 0. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 15 December 2010 (MN LATEX style file v2.2). A general model of resonance capture in planetary systems:First and second order

  5. Collisional Evolution of Irregular Satellite Swarms: Detectable Dust…

    https://people.ast.cam.ac.uk/~wyatt/kw11.pdf
    25 Nov 2010: arX. iv:1. 011. 4858. v1 [. astr. o-ph. EP]. 22. Nov. 201. 0Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 November 2010 (MN LATEX style file v2.2). Collisional Evolution of Irregular Satellite Swarms:. Detectable Dust around Solar

  6. Are Debris Disks Self-Stirred?

    https://people.ast.cam.ac.uk/~wyatt/kw10.pdf
    19 Feb 2010: When stirring reachesthe outer edge, all disks break to a faster decline in fbecause no new regions can be stirred.

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