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1 - 8 of 8 search results for scholarships 2022 |u:people.ast.cam.ac.uk where 0 match all words and 8 match some words.
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  2. Academic CV

    https://people.ast.cam.ac.uk/~lr439/CV.html
    21 Oct 2023: 2022-Present. Research Focus: Using polluted white dwarfs to constain the bulk composition of exoplanetary material. ... Committee member: International Women's Day Committee Institute of Astronomy, University of Cambridge (2022 - present).
  3. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: 2022 The Authors. arX. iv:2. 307. 0157. 4v1. [as. tro-. ph.E. ... 2022). Whilst heating from thestar can lead to release of CO (Kral et al.
  4. Submission_HoC_NWE

    https://people.ast.cam.ac.uk/~nwe/Culture.pdf
    11 Oct 2023: blog/2022/11/02/guest-post-the-bullying-of-hannelore/. [9]
  5. About Me

    https://people.ast.cam.ac.uk/~lr439/About_Me.html
    21 Oct 2023: From October 2022 I began a postdoc at the Institute of Astronomy, University of Cambridge, UK where I am able to continue my studies of white dwarf planetary systems.
  6. TOPICS IN ASTROPHYSICS Much astrophysical research is…

    https://people.ast.cam.ac.uk/~wyatt/topics1.pdf
    29 Sep 2023: Number expected to detect brighter than is. Exam question from 2022:. ... Total flux per square degree. Exam question from 2022:. For a Poisson distribution with mean , a number of occurrences occurs with probability.
  7. MNRAS 000, 1–11 (2023) Preprint 31March 2023 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/mmcb23.pdf
    31 Mar 2023: 2021;Najita et al. 2022). Theinheritance of structure from the protoplanetary to debris disc phaseis still uncertain (Lodato et al. ... 2020; Hales et al. 2022), but more recentlyalso later type stars (Matrà et al.
  8. The clumpy structure of epsilon Eridani's debris disc revisited…

    https://people.ast.cam.ac.uk/~wyatt/bpkw23.pdf
    27 Mar 2023: Accepted 2023 March 23. Received 2023 March 7; in original form 2022 April 12. ... 2022). 3h32m56s 54s 52s. -926'40". 27'00". 20". 40". 28'00". RA. Dec.
  9. MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yw23.pdf
    29 Sep 2023: 2015; Han et al. 2022) as well as N-bodysimulations of mutual planetesimal scattering (Ida & Makino 1992),though in our model a companion star is perturbing the disc so thecharacteristic eccentricity ... 2021). Γ = 2.92(𝐿𝐿. )0.13, (26). and, for

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