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1 - 10 of 30 search results for KaKaoTalk:ZA31 24 24 |u:people.ast.cam.ac.uk where 0 match all words and 30 match some words.

  1. Results that match 2 of 3 words

  2. MNRAS 000, 1–17 (2022) Preprint 28 June 2022 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf
    22 Mar 2024: 𝑡vis =. 𝜋𝑟Δ𝑟. 3︁2ln(2)𝜈. 𝑟Δ𝑟2𝜈. (24). With this definition, the steady-state surface density ( ¤𝑀+/(3𝜋𝜈)) isindependentofΔ𝑟,andmatchesthesurfacedensityobtainedsolvingthe radial viscous evolution and the

  3. Prof Richard McMahon, Institute of Astronomy, Cambridge Home Page

    https://people.ast.cam.ac.uk/~rgm/
    1 Jun 2024: Tel: 44-(0)-1223-337519/337548. FAX: 44-(0)-1223-337523. Last modified: Sat Jun 1 12:46:24 BST 2024.

  4. 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.

  5. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/Astro-jobs_1_2308.pdf
    15 Aug 2023: 15/08/2023 24. Non Astronomy Jobs? Transferable skills.  Problem solving Creative thinking Self motivating and managing Analytic/computing/numerical experience/skills.

  6. MNRAS 000, 1–24 (2023) Preprint 9 November 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/pksj23.pdf
    22 Mar 2024: MNRAS 000, 1–24 (2023). The effect of planets on debris-disc edges 3. ... MNRAS 000, 1–24 (2023). 4 T. D. Pearce et al. Figure 2.

  7. 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.

  8. 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.

  9. 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.

  10. Draft version March 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: Draft version March 24, 2022Typeset using LATEX twocolumn style in AASTeX63.

  11. Draft version July 18, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: 2019) show 24 µm excesses, as dust production declines with time due to collisional. ... The last column lists. the 24 µm excess ratio (Fobs/Fstar) determined by Sierchio et al.

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