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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.

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.

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.

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

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.

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.

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.