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1 - 10 of 13 search results for KaKaoTalk:ZA31 24 24 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

  1. Results that match 2 of 3 words

  2. Table of Contents 2 Tides Locally familiar 2.1 Astrophysical ...

    https://people.ast.cam.ac.uk/~wyatt/topics2.pdf
    29 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.

  3. Lecture09_slides

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture09_slides.pdf
    28 Oct 2023: 4. 5. 6. 7. temperature. luminosity. opacity. 15 Msun. All models for X = 0.74, Y = 0.24.

  4. TOPICS IN ASTROPHYSICS Much astrophysical research is…

    https://people.ast.cam.ac.uk/~wyatt/topics1.pdf
    29 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.

  5. Lecture06

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture06_slides.pdf
    17 Oct 2023: log(A f ). bmicro (km s1). 24/06/2011 16:38Curves of growth: metallicity and vt.

  6. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture09.pdf
    28 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.

  7. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture03.pdf
    10 Oct 2023: 4. The average EV I for the cluster is approximately 0.24 in this plot.

  8. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf
    23 Oct 2023: Eit =(E0ρ. )rit. erg s1 cm3. g cm3 erg s1 g1 (7.24).

  9. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture11.pdf
    6 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).

  10. MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/mmcb23.pdf
    31 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

  11. The clumpy structure of epsilon Eridani's debris disc revisited…

    https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf
    27 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

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