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Submission_HoC_NWE
https://people.ast.cam.ac.uk/~nwe/Culture.pdf11 Oct 2023: This puts an unfair economic bias on the success of academic careers, which is again detrimental to diversity of ideas and people. ... It would be very helpful to obtain statistics on socio-economic backgrounds in Astronomy, both for professional -
Planetary System DynamicsPart III Mathematics / Part III Astrophysics …
https://people.ast.cam.ac.uk/~wyatt/psd_eg4.pdf20 Nov 2023: 1. 2. Test particle evolution / secular resonancesThe orbits of test particles in a planetary system evolve due to the secular perturbations of planets whoseorbits also evolve due to their mutual perturbations. ... a) Consider a test particle in the two -
Planetary System DynamicsPart III Mathematics / Part III Astrophysics …
https://people.ast.cam.ac.uk/~wyatt/psd_eg2.pdf5 Nov 2023: 1/3, have a period. 2πµ1(43α). 2. 3. Tadpole and horseshoe orbitsThe equations of motion of a test particle in the circular restricted three body problem expressed in polarcoordinates in ... 3. 4. Patched conic sections / resonance overlapConsider -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/Astro-jobs_1_2308.pdf15 Aug 2023: students at the IoA [DAMTP/Physics] you are not fair test particles. -
Lecture13_slides
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture13_slides.pdf14 Nov 2023: It is with this idea inmind that Bergeron, Saffer, & Liebert (1992, BSL hereafter) decided to test thespectroscopic method using DA white dwarfs at higher effective temperatures(Teff > 13, 000 K) where -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture09.pdf28 Oct 2023: In neglecting this slight asymmetry, we make the assumptionthat the additional centripetal force acting on a test mass at the equatorof the star is small compared to the gravitational force. -
The clumpy structure of epsilon Eridani's debris disc revisited…
https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf27 Mar 2023: Observations over multipleepochs are necessary to test whether the observed features rotate around the star. ... We first test this processwith the original unsmoothed data and confirm that we mea-. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture02.pdf10 Oct 2023: Gaia is also providing a numberof stringent new tests of general relativity and cosmology. -
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. -
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 -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf24 Nov 2023: This is fundamental work, providing empirical tests ofour theories of stellar evolution for massive stars.
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