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11 - 18 of 18 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 18 match some words.

  1. Results that match 1 of 2 words

  2. Astronomy & Astrophysics manuscript no. SHARDDS Β©ESO 2022August…

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: This detection rate re-quires the successive injection of 20 fake companions per con-sidered annulus. ... We relied on ten particles with a maximum number ofiterations equal to 20.

  3. Inner edges of planetesimal belts: collisionally eroded or truncated?

    https://people.ast.cam.ac.uk/~wyatt/immb23.pdf
    20 Feb 2024: Accepted 2023 April 21. Received 2023 April 20; in original form 2022 September 9. ... nloaded from https://academ. ic.oup.com/m. nras/article/522/4/6150/7143114 by guest on 20 February 2024.

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

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: 20. 30. Du. st-t. o-G. asR. atio. Gas Density. Dust Density. ... The dusttemperature also affects the timescales relevant for grainalignment, but the 20% difference is inconsequential (seeSection 8).

  5. MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/hwd22.pdf
    22 Mar 2024: 7 Ja. n 20. 23. 2 Han et al. depends on the relative fractions of planetesimals in each differenttype of resonance (Wyatt 2003). ... Median 1𝜎 2𝜎 3𝜎. Linear displacement speed (au/yr) 0.018 (-0.099, 0.13) (-0.29, 0.33) (-0.86, 0.90)Location atMJD

  6. Astronomy & Astrophysics manuscript no. main Β©ESO 2023October 11, …

    https://people.ast.cam.ac.uk/~wyatt/dmch23.pdf
    22 Mar 2024: 5 10 15 20. Distance from the Sun (pc). 0.2. 0.4. ... 5. 10. 15. 20. 25. MK. 1(m. ag). (1). (3). M0-M5.

  7. 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

  8. 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).

  9. 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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