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1 - 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. Prof Richard McMahon, Institute of Astronomy, Cambridge Home Page

    https://people.ast.cam.ac.uk/~rgm/
    28 Jun 2024: Strabane had moved out of the top 20 in the 2008 edition.".

  3. Erin E Hayes

    https://people.ast.cam.ac.uk/~eeh55/resume.html
    2 May 2024: Presented “The Fate of the Universe” talk to three groups of 20 Year 5 (Ages 9-10) students.

  4. Mark Wyatt

    https://people.ast.cam.ac.uk/~wyatt/
    10 Jul 2024: The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 Micron Spectrum of the Planetary-Mass Companion VHS1256-1257b.

  5. Astronomy & Astrophysics manuscript no. aa ©ESO 2024April 9, ...

    https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf
    9 Apr 2024: 0. 20. 40. 60. 80. 100. Inte. nsity. (%). ALMA-NEALMA-SWHerschel70-NEHerschel70-SWmodel profile-ALMA beammodel profile-Herschel70 beamALMA beam sizeHerschel70 beam size. ... Using equation (20)in Wyatt et al. (2007) and assuming the warm component

  6. Draft version July 18, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: 2010), the Spitzer 70 µm observations of a subsample of 20 systems (red, Stauffer et al. ... µm (20′′) clearly encompass any circumstellar dust emission around Pleiades members but also raise the spectre of.

  7. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: Figure 1: Molecules relevant to terrestrial planet characterization between 3-20 μm (adapted from Catling et al. ... In the following we will summarize what developments from ground and space we can expect in the coming 20 years.

  8. Cosmic dust fertilization of glacial prebiotic chemistry on early ...

    https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf
    22 Mar 2024: Nonetheless, even Dry Valleys type cryoconite deposits are subject to transportthrough ice dynamics of up to 20 m/yr [41], precluding long-term formations. ... Origins of Life and Evolution of Biospheres 38, 5–21(2008). [20] Maurette, M., Hammer, C.,

  9. 2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…

    https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf
    22 Mar 2024: to 20 Micron Spectrum of the Planetary-Mass Companion VHS 1256-1257 b. ... MIRI Channel 4, Short A 17.71 - 20.94 FULL FASTR1 1,460 – 1,930 1576.22.

  10. MNRAS 000, 1–17 (2023) Preprint 25 October 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: The 𝛽 PictorisMoving Group (BPMG) is both young (20 Myr, Bell et al. ... 36 0.908 -V WW PsA 35 20 78 0.908 -AU Mic - 110 13000 - 40.

  11. MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf
    22 Mar 2024: ph.E. P] 1. 6 Ju. n 20. 23. 2 James Terrill et al. ... 𝜎𝑟 (au) ⟨𝑖⟩ (). 0.01 5 89.31.00.50.01 10 89.21.20.20.01 20 89.61.20.40.03 5 89.61.30.50.03 10

  12. 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.

  13. 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.

  14. 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).

  15. 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

  16. 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.

  17. 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

  18. 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).

  19. 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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