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M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf23 Oct 2023: Referring to Figure 7.1, the gravitational force acting on a test particle ofmass dmi at a distance r from the centre of a spherically symmetric massdistribution is. ... The corresponding gravitational potential energy ofthe test mass is:. dUg,i = GMr dmi -
MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf11 Jul 2023: potential test for. ... order of magnitude.This is plausibly an important test of whether large planetes-imals. -
Draft version March 24, 2022Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf22 Mar 2024: We performour averaging tests using different sections (e.g., quarters,thirds, halves) of a box that is slightly longer than theone used for the full-disk averaging described above. ... from the outer regions of the disk, our second test is toanalyze the -
MNRAS 000, 1–24 (2023) Preprint 9 November 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/pksj23.pdf22 Mar 2024: so we can test different initial surface-density profiles; weconsider initial surface-density profiles between 𝑟0 and 𝑟1.5. -
Cosmic dust fertilization of glacial prebiotic chemistry on early ...
https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf22 Mar 2024: This minimises sources of uncertainty thatwould otherwise be difficult or impossible to constrain, i.e., allowing us to test theprebiotic relevance of dust supply in one well constrained early Earth scenario. -
MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/yw23.pdf29 Sep 2023: observations. This paper aims to test how often the action of the Kozai-Lidovmechanism on a belt of planetesimals due to a wide binary compan-ion can excite the largest planetesimals ... Figure 3. Evolution of a test particle in the eccentric Kozai-Lidov -
Quanz_et_al_ESA_white_paper_MIR_interferometry_revised
https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf22 Mar 2024: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact -
Draft version July 18, 2022Typeset using LATEX default style ...
https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf22 Mar 2024: Withthese assumptions, we can test if the same evolutionary model is consistent with observations of the Pleiades. -
Inner edges of planetesimal belts: collisionally eroded or truncated?
https://people.ast.cam.ac.uk/~wyatt/immb23.pdf20 Feb 2024: We use both parametric and non-parametric modelling to test if their inner edges are shallow and consistent with collisional evolution. -
Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…
https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf22 Mar 2024: The PSO framework was chosen as it showed, during tests,a higher convergence rate than Bayesian optimisation and al-lowed multi-core estimation7, reducing the computation time.More standard minimisation frameworks
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