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Planetary System DynamicsPart III Mathematics / Part III Astrophysics …
https://people.ast.cam.ac.uk/~wyatt/psd_eg1.pdf29 Sep 2023: e) Derive an expression for the distance of the particle P from the geometric centre of the ellipse O, andhence show that to first order in eccentricity the distance OP is -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture02.pdf10 Oct 2023: Magnitudes andluminosities are normally measured through a given filter; Figures 2.4 and2.5 show the transmission curves of some of the most commonly used op-tical and near-infrared filters. -
https://people.ast.cam.ac.uk/~vasily/data/TAP_1697550531535.vot
https://people.ast.cam.ac.uk/~vasily/data/TAP_1697550531535.vot17 Oct 2023: ARI's TAP access to the Gaia Archive. Unique source identifier (unique within a particular Data Release) Basis function coefficients for the BP spectrum representation Basis function coefficients for the RP spectrum representation -
MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled…
https://people.ast.cam.ac.uk/~wyatt/mmcb23.pdf31 Mar 2023: MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled usingMNRASLATEXstyle file v3.0. Stirred but not shaken: a multi-wavelength view of HD 16743’s debris disc. JonathanP.Marshall,1,2 J.Milli,3 E.Choquet,4 C. delBurgo,5 G.M.Kennedy,6,7 F.Kemper,8
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