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1 - 10 of 17 search results for katalk:za33 24 |u:people.ast.cam.ac.uk where 0 match all words and 17 match some words.

  1. Results that match 1 of 2 words

  2. https://people.ast.cam.ac.uk/~bothwell/Files/LICENSE.txt

    https://people.ast.cam.ac.uk/~bothwell/Files/LICENSE.txt
    17 May 2024: on July 24, 1971).

  3. 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.

  4. 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.

  5. 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.

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

    https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf
    9 Apr 2024: 2016)found a significant warm excess at 24 µm of Spitzer/MIPS basedon the Dodson-Robinson et al. ... The beam size is represented by a white ellipse (left: 2.24′′ 1.84′′, middle: 2.28′′ 1.89′′, right: 1.43′′ 1.12′′) inthe

  7. Mark Wyatt

    https://people.ast.cam.ac.uk/~wyatt/
    15 Apr 2024: J., Stapelfeldt K. R., Wyatt M. C. 2015, ApJS, 216, 24.

  8. 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.

  9. 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

  10. 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

  11. 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

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