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The clumpy structure of epsilon Eridani's debris disc revisited…
https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf27 Mar 2023: process. In this simulation, a 0.2 MJ planet has migrated out-wards from 37 au at 0.2 au Myr1 for 24 Myr, while interact-ing with a disc with -
MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/yw23.pdf29 Sep 2023: 𝑀bb = 1.75 107𝑅13/3bb 𝑡. 1oct𝑀mid, (24). where 𝑀bb and 𝑀mid are in 𝑀, 𝑅bb is the black body radius of thebelt in au and 𝑡oct is in Myr. ... This is why the blackbodyradius is used in equation 24 and the belt mass is correct -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf24 Nov 2023: 24. and their evolution, Chevalier and collaborators showed that they occurin sheets of dust (and gas) located 120 and 330 pc in front of thesupernova, and that the dust producing the -
MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf11 Jul 2023: ṁrv,k = χrk(fv,k)mv,kR. rk. (24). 2.5 Release of CO following collisions. -
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
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