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arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...
https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf29 Apr 2016: arX. iv:1. 604. 0828. 6v1. [ast. ro-p. h.E. P]. 28 A. ... by high orbital eccentricity comets,is likewise difficult to achieve from a dynamical perspective. -
Space Science Reviews manuscript No.(will be inserted by the ...
https://people.ast.cam.ac.uk/~wyatt/wj16.pdf15 Mar 2016: 2007), but could have a dramatic effect on the emission spectrum of theplanet. ... Typically the total mass of debris created in a giant impact iswell known. -
arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf7 Oct 2016: The origin of this hot dust is a matter of consid-erable debate. ... Nevertheless,a growing number of systems host planets and debris(Wyatt et al.
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