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19 Apr 2006: The collision rate (bottom) is the product of the volume densityof cross-sectional area of planetesimals (top) and the relative ve-locity of collisions (middle). ... This has the potential to provide a valu-able observational test of models which explain

11 Jul 2019: However, us-ing a Kolmogorov-Smirnov (KS) test, they demonstratedthat the period distributions of their disc-bearing anddisc-free binaries and multiples were not, in fact, differ-ent in a statistically ... Theupper, middle and lower panels show

7 Jul 2020: Future imaging ofthe faint debris disc in π Men and precise constraints on the stellar spin orientationwould provide strong tests for these formation scenarios.

5 Oct 2012: 70µm images on the left, 100µm images in the middle and 160µm onthe right. ... 70µm images are on the left,100µm images in the middle and 160µm on the right.

23 Oct 2012: The non-unique nature of the spectral modeling allows us to test additional PSDs that can. ... Figure 6. middle shows a broken power law, with below 1 μm and.

16 Nov 2011: We test the goodness of these analytical approxima-tions by considering a close-in planet (at a0 = 2 AU) inthe robustly runaway regime of a supernova.

14 Feb 2022: We also test a different more physically moti-vated model for releasing the CO and assume it comes from theslow heating provided by the Sun over long timescales, whichwarms up large ... 2017, 2019) is valid for the KB (Model 1).Second, we test a more

2 Nov 2015: Asymmetric dips with lagging tails (middle)or complex structures (bottom) are clearly non-planetary. ... Phase. 2.46 d. Figure 4. Examples of quasi-periodic (top, middle) and aperiodic (bottom) dippers.

10 Feb 2014: nity to test theoretical models and to piece together the story of planetary systems. ... ometric tests using various permutations of a model consisting of a central source encircled by.

24 Nov 2023: This is fundamental work, providing empirical tests ofour theories of stellar evolution for massive stars. ... Middle pair: SN2005cs in M51 ata distance of 7 Mpc. Bottom pair: SN2003gd in the face-on spiral galaxy M74 at adistance of 9 Mpc.

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.

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.

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

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