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Table of Contents 2 Tides Locally familiar 2.1 Astrophysical ...
https://people.ast.cam.ac.uk/~wyatt/topics2.pdf29 Sep 2023: Mr0 IMr. 24 Mz MrKM1. Mr M. z=M2)/a3. CM2/nZ = am,/[a-x]2. & ... 2,42,4 24 L5. stabilisedby Coriolis fores. 24,25 14. Jupiter. 2.6 Outcomes of Close Encounters. -
Lecture09_slides
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture09_slides.pdf28 Oct 2023: 4. 5. 6. 7. temperature. luminosity. opacity. 15 Msun. All models for X = 0.74, Y = 0.24. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/Astro-jobs_1_2308.pdf15 Aug 2023: 15/08/2023 24. Non Astronomy Jobs? Transferable skills. Problem solving Creative thinking Self motivating and managing Analytic/computing/numerical experience/skills. -
TOPICS IN ASTROPHYSICS Much astrophysical research is…
https://people.ast.cam.ac.uk/~wyatt/topics1.pdf29 Sep 2023: of considering populations of astrophysical objects as distributions. Lectures 13 - 24 : Planet Formation and Evolution (Oli Shorttle). ... Vanables.a[my], M [M], BY. To maintain wrR0 =aM/R8.= =24(n =2πvtam. Taynvain. -
Lecture06
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06_slides.pdf17 Oct 2023: log(A f ). bmicro (km s1). 24/06/2011 16:38Curves of growth: metallicity and vt. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture09.pdf28 Oct 2023: at r = 0 (9.24). Physically, this is simply saying that there isn’t a core of infinite densityor negative luminosity at the centre of a spherically symmetric star. ... 7. temperature. luminosity. opacity. 15 Msun. All models for X = 0.74, Y = 0.24. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture03.pdf10 Oct 2023: 4. The average EV I for the cluster is approximately 0.24 in this plot. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf23 Oct 2023: Eit =(E0ρ. )rit. erg s1 cm3. g cm3 erg s1 g1 (7.24). -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture11.pdf6 Nov 2023: 11.24). Note that the free-fall timescale is independent of the initial radius of thesphere, and depends only on the initial density ρ0. ... One such evolutionary track is givenapproximately by:. log L = 10 log M 7.24 log Teff C (11.37). -
MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled…
https://people.ast.cam.ac.uk/~wyatt/mmcb23.pdf31 Mar 2023: 0.44 5625 51 Johnson 𝐵 Høg20000.55 7047 66 Johnson𝑉 Høg20000.64 6808 62 Gaia 𝐺 GaiaDR30.78 7146 66 Cousins 𝐼 Wu20131.24 5544 132 2MASS 𝐽 Skrutskie ... Moór 2015160 174 24 Spitzer MIPS Moór 2011160 226 32 Herschel PACS Moór 2015250 82 -
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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