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  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. 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. 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.
  5. 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.
  6. 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.
  7. 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.
  8. 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.
  9. 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.
  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. Mark Wyatt

    https://people.ast.cam.ac.uk/~wyatt/
    15 Apr 2024: J., Stapelfeldt K. R., Wyatt M. C. 2015, ApJS, 216, 24.
  12. 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.
  13. Astronomy & Astrophysics manuscript no. aa ©ESO 2024April 9, ...

    https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf
    9 Apr 2024: 2016)found a significant warm excess at 24 µm of Spitzer/MIPS basedon the Dodson-Robinson et al. ... The beam size is represented by a white ellipse (left: 2.24′′ 1.84′′, middle: 2.28′′ 1.89′′, right: 1.43′′ 1.12′′) inthe
  14. 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.
  15. Astronomy & Astrophysics manuscript no. SHARDDS ©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: 1HD 9672 01:34:38 -15:40:34 5.61 5.53 A1V 406 57.08 1HD 10472 01:40:24 -60:59:56 7.61 6.69 F2IV/V 307 ... 409 45.60 1HD 14082B 02:17:25 28:44:30 7.74 6.36 G2V 219 39.75 1AG-Tri 02:27:29 30:58:24 10.12 7.24
  16. 22 Mar 2024: 9 Fe. b 20. 24. that localised sedimentary deposits of cosmic dust could have accumulated in aridenvironments on early Earth – in particular glacial settings that today producecryoconite sediments.
  17. 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).
  18. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 2018) and 24% of A-typestars (Thureau et al. 2014), but only detected two excesses aroundM-types (GJ 581; Fomalhaut C; Lestrade et al. ... 46 15.0 - 313.7 7.0 31.05.18 0.8 J0141-0928, J0006-0623BD30 397 B 30.47 44 15.1 - 500.2 5.6 24.08.18
  19. 22 Mar 2024: 0613. 3920. 18-1. 1-24. H23. HD. 9949. 220. 18-0. 2-03. H23. ... BD. 0613. 3920. 18-1. 1-24. H23. HD. 9949. 220. 18-0. 2-03.
  20. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact
  21. 2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…

    https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf
    22 Mar 2024: Stapelfeldt ,22. Jordan M. Stone ,23 Jason J. Wang ,24, 25 Olivier Absil ,26 William O. ... MIRI Channel 4, Medium B 20.69 - 24.44 FULL FASTR1 1,680 – 1,770 1576.22.

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