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31 - 33 of 33 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 33 match some words.

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  2. 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.

  3. MNRAS 000, 1–16 (2022) Preprint 6 July 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/bwmd23.pdf
    11 Jul 2023: 20 of Wyatt et al. (2011), where δis now the spacing between mass bins and not radial bins,ηmax = 1/2, such that α. ′ = ... Σk=ilrF(k i) = 1. (20). In a similar manner, the rate of mass gain for volatiles isgiven by :. ṁcv,k = Σimki=1 Fv(k i,

  4. https://people.ast.cam.ac.uk/~vasily/data/TAP_1697550531535.vot

    https://people.ast.cam.ac.uk/~vasily/data/TAP_1697550531535.vot
    17 Oct 2023: 62a4UsB2iLNKl45QFu5p7QCEPbASplqEJsu7EA2luUOFsIQDHV1IWs7WNAAK7O tCxqcUATVmbH2iBKwDgUkfNfFw1AByAenwCtEcAhtROsYFNOP/sVFTy9nI/wkB lyCBskARZxNuZuefv/zU368oWzA/64r94GHkML/m3wwXTlx6Pdk5zEEKS/ucCM

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