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11 - 13 of 13 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

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  2. DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/srw23.pdf
    22 Mar 2024: 2018; Wyatt2020). To date, such exo-Kuiper belts, or debris disks, havebeen detected around 20% of nearby main-sequence starsthrough their excess emission at infrared wavelengths (Mon-tesinos et al. ... with a power-law in-dex of p = 1 with ain = 30 au

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

    https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf
    22 Mar 2024: ph.E. P] 2. 7 Ju. n 20. 22. 2 S. Marino. ... 𝑅ion,0 =. πœ™πœ†πœŽCI dπœ†, (20). andcorrespondstoanionisationtimescaleof100yr.Recombinationis calculated as. 𝑅rc(𝑧) = 𝛼rc(𝑇)𝑛e (𝑧), (21).

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

    https://people.ast.cam.ac.uk/~wyatt/pksj23.pdf
    22 Mar 2024: such dust is detected around 20% of main-sequence stars(Hughes et al. ... Each simulation comprises one star, one planet,and a disc of 20,000 massless debris particles.

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