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1 - 10 of 13 search results for :pc53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 13 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: MNRAS 000, 1–24 (2023). The effect of planets on debris-disc edges 3. ... MNRAS 000, 1–24 (2023). 4 T. D. Pearce et al. Figure 2.

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

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: Draft version March 24, 2022Typeset using LATEX twocolumn style in AASTeX63.

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

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: 2019) show 24 µm excesses, as dust production declines with time due to collisional. ... The last column lists. the 24 µm excess ratio (Fobs/Fstar) determined by Sierchio et al.

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

    https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf
    22 Mar 2024: 9 Fe. b 20. 24. that localised sedimentary deposits of cosmic dust could have accumulated in aridenvironments on early Earth – in particular glacial settings that today producecryoconite sediments.

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

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: 1HD 9672 01:34:38 -15:40:34 5.61 5.53 A1V 406 57.08 1HD 10472 01:40:24 -60:59:56 7.61 6.69 F2IV/V 307 ... 409 45.60 1HD 14082B 02:17:25 28:44:30 7.74 6.36 G2V 219 39.75 1AG-Tri 02:27:29 30:58:24 10.12 7.24

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

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 2018) and 24% of A-typestars (Thureau et al. 2014), but only detected two excesses aroundM-types (GJ 581; Fomalhaut C; Lestrade et al. ... 46 15.0 - 313.7 7.0 31.05.18 0.8 J0141-0928, J0006-0623BD30 397 B 30.47 44 15.1 - 500.2 5.6 24.08.18

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

    https://people.ast.cam.ac.uk/~wyatt/mcjm22.pdf
    22 Mar 2024: 𝑡vis =. 𝜋𝑟Δ𝑟. 3︁2ln(2)𝜈. 𝑟Δ𝑟2𝜈. (24). With this definition, the steady-state surface density ( ¤𝑀+/(3𝜋𝜈)) isindependentofΔ𝑟,andmatchesthesurfacedensityobtainedsolvingthe radial viscous evolution and the

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

    https://people.ast.cam.ac.uk/~wyatt/dmch23.pdf
    22 Mar 2024: 0613. 3920. 18-1. 1-24. H23. HD. 9949. 220. 18-0. 2-03. H23. ... BD. 0613. 3920. 18-1. 1-24. H23. HD. 9949. 220. 18-0. 2-03.

  10. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb22.pdf
    22 Mar 2024: 1. Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity. Corresponding author: Sascha P. Quanz, ETH Zurich, Institute for Particle Physics and Astrophysics, Zurich, Switzerland Contact

  11. 2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…

    https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf
    22 Mar 2024: Stapelfeldt ,22. Jordan M. Stone ,23 Jason J. Wang ,24, 25 Olivier Absil ,26 William O. ... MIRI Channel 4, Medium B 20.69 - 24.44 FULL FASTR1 1,680 – 1,770 1576.22.

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