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1 - 10 of 11 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 11 match some words.

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

    https://people.ast.cam.ac.uk/~wyatt/swmw22.pdf
    22 Mar 2024: collisional evolution. Only 6 systems with ages in the range 50 to 200 Myr were detected. ... The typical FWHM beam size of 1.′′5 (200 au) comfortably encompasses dust belts with radii up to 100 au.

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

    https://people.ast.cam.ac.uk/~wyatt/ckkl23.pdf
    22 Mar 2024: 200. 0. 200. 400. µJy. /Bea. m. Figure 1. Naturally weighted ALMA 880𝜇m images of our BPMG M-dwarf sample. ... 0. 200. 400. µJy. /Bea. m. Figure 2. Naturally weighted ALMA 880𝜇m image of TYC 7443-1102-1.The stellar location is marked with a.

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

    https://people.ast.cam.ac.uk/~wyatt/dmac22.pdf
    22 Mar 2024: 2009), we removed the contrast at 200 and 700 mas, whichled to multicollinearity, affecting potentially the definition of theclusters. ... 200 400 600 800 1000Radial distance (mas). 10 6. 10 5.

  5. Mark Wyatt

    https://people.ast.cam.ac.uk/~wyatt/
    15 Apr 2024: being accreted onto the Earth is in grains between 100-200 micron in size is understood in terms of the interplay between Poynting-Robertson drag and collisions, this result has not

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

    https://people.ast.cam.ac.uk/~wyatt/ylkw24.pdf
    9 Apr 2024: 2.36 0.21 2.40 0.16 2.41 0.16Fc(µJy) Flux at stellar position 183 14 183 15 198 30 200 31 184 16 184 16PA() disc position ... 0 25 50 75 100 125 150 175 200 225 250 275Radius (AU).

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

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: 6 Hull et al. 200 100 0 100 200Position along major axis (au).

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

    https://people.ast.cam.ac.uk/~wyatt/wrll24.pdf
    22 Mar 2024: Cosmic dust fertilization of glacial prebiotic. chemistry on early Earth. Craig R. Walton1,2, Jessica K. Rigley2, Alexander Lipp3,Robert Law4, Martin D. Suttle5, Maria Schönbächler1,. Mark Wyatt2, Oliver Shorttle2,6. 1Department of Earth Sciences

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

    https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf
    22 Mar 2024: A case of a double Gaussian radial distribution, with = 0.03and 𝜎𝑟 = 20 au, peaking at 100 au and 200 au, shown in the middlepanel of Figure 2. • ... 0.06 0.08 0.10 0.12 0.14. h. 600. 500. 400. 300. 200.

  10. DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/srw23.pdf
    22 Mar 2024: DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style in AASTeX631. Formation of Gaps in Self-gravitating Debris Disks by Secular Resonance in a Single-planet System. II. Towards aSelf-consistent Model. ANTRANIK A. SEFILIAN,1, 2 , ROMAN R.

  11. 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

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