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24 Apr 2007: 30. Wavy size distributions: middle/top. The transition from strength to gravity scaling also causes a wave in the size distribution. • ... be used to test models. …

24 Nov 2012: Hence, we conclude that this test rejects the possibility thatthe superposition of two background point sources can be re-sponsible for the central emission. ... 2011) (see also Sibthorpe et al. (2012)). Second,the spectra of these test sources removed

22 Nov 2018: which we will test further by comparing to models inthe next subsection 4.2.

18 Aug 2020: We also discuss potential tests toconstrain the largest planetesimal sizes and debris disc masses. ... Inter-estingly, the opacity 1.7 cm2 g1(850 µm/λ) assumed here,or 1.45 cm2 g1 at 1 mm, is in the middle of the range forthese extreme assumptions.

21 Feb 2019: 13CO emission (middle panel) is alsobrighter in the southwest for as far as 2.′′8, beyond whichthe northeast of the disc is brighter. ... 5.3.2 Temperature Scenario. To test the possibility of temperature variation as the causeof asymmetry in the

5 Jul 2011: Mon. Not. R. Astron. Soc. 000, 1–20 (2010) Printed July 5, 2011 (MN LATEX style file v2.2). Multi-Wavelength Modelling of the β Leo Debris Disc: 1, 2 or 3planetesimal populations? L J Churcher 1†, M.C. Wyatt1, G. Duchêne2,3, B. Sibthorpe4, G.

15 Mar 2016: a stable Laplace resonance, in theSaturnian system they became unstable and collided, with the present middle-sized moons representing the remnants of this former satellite population. ... Debris particles are massless test particles, and no accountis

23 Dec 2017: These re-sults advocate for additional tests with the various proposedcircumstellar scenarios in order to resolve whether the dy-namical history of such material could produce the shapes ofthe dips. ... In the middle of SkaraBrae (on UT 2017 August 8; JD

30 Jan 2004: It was also unclear whether the real cryostat had been used for the thermal cycling tests or a test cryostat. ... exist. There was then some general discussion regarding the laboratory and commissioning tests.

8 Jul 2008: Dynamics of small bodies in planetary systems. Mark C. Wyatt. Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA, UKwyatt@ast.cam.ac.uk. The number of stars that are known to have debris disks is greater than thatof stars known to