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21 - 30 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. Astronomy & Astrophysics manuscript no. SHARDDS ©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. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture16.pdf
    24 Nov 2023: 2003ie a. b. 1999an2002hh1999ev1999br1999em2001du2004dj1999gi. 2006my2007aa2004am2004dg2006bc2006ov2004et2008bk2005cs2003gd2004A. 2019181716151413121110987654321. 5. 25. 20. 15. 5 6 7 8 9 10. ... Thetypical energies of the ν̄e were 20 MeV. Neutrinos

  4. 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.

  5. 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).

  6. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture11.pdf
    6 Nov 2023: 11.19 can in turn be re-written as. cos2 ξdξ. dt=χ. 2(11.20). ... 20. ionisation potential IP = 13.6 eV) in the surrounding interstellar medium,producing an H ii region around the star(s).

  7. 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

  8. Astronomy & Astrophysics manuscript no. main ©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.

  9. 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

  10. 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 =. 𝜙𝜆𝜎CI d𝜆, (20). andcorrespondstoanionisationtimescaleof100yr.Recombinationis calculated as. 𝑅rc(𝑧) = 𝛼rc(𝑇)𝑛e (𝑧), (21).

  11. MNRAS 000, 1–22 (2021) Preprint 29 September 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/yw23.pdf
    29 Sep 2023: P] 2. 8 Se. p 20. 23. 2 S. D. Young and M. ... 𝑛(𝐷) = 𝐾𝐷𝛼, (20). where 𝛼 is 3.5 in an infinite collisional cascade (Dohnanyi 1969)and K is a normalisation constant.

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