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

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  2. M. Pettini: Introduction to Cosmology — Lecture 15 CLUSTERS ...

    https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture15.pdf
    28 Jun 2020: The thresholdδvirnonlin ' 200 is often used to define a collapsed object. ... The ‘virial’ radius isthe radius around a structure (a galaxy, a cluster) within which the densityis ' 200 times higher than the average background density.

  3. MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/aght19.pdf
    17 Jan 2020: MNRAS 000, 1–19 (2019) Preprint 20 December 2019 Compiled using MNRAS LATEX style file v3.0. Are Inner Disc Misalignments Common? ALMA Reveals an IsotropicOuter Disc Inclination Distribution for Young Dipper Stars. M. Ansdell,1,2,3? E. Gaidos,4 C.

  4. Draft version March 10, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/edhm20.pdf
    10 Mar 2020: 0.1 0.3 1.0 3.0 10.0Age [Gyr]. 200. 0. 200. 400. 600.

  5. MNRAS 000, 1–20 (2020) Preprint 18 August 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/kw20.pdf
    18 Aug 2020: cade (q = 3.5) in the size range from 1 mm to 200 km. ... their formation with qbig = 2.8 up to a size of 200 km.

  6. Draft version June 29, 2020Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mdwm20.pdf
    29 Jun 2020: a steep inner edge (at 60-80 au). The belt is very broad, extending out to at least 150-200 au.

  7. MNRAS 000, 1–22 (2019) Preprint 30 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mfhk20.pdf
    30 Jan 2020: The carbon finalsurface density, on the other hand, is very similar for bothscenarios, with differences only beyond 200 au.

  8. MNRAS 000, 1–7 (2019) Preprint 28 January 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mwkk19.pdf
    28 Jan 2020: 2015) and an opacity that declines with wavelength as 1/λbeyond 200 µm (Wyatt 2008).

  9. MNRAS 000, 1-30 (2020) Preprint 12 October 2020 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/swmn20.pdf
    15 Oct 2020: MNRAS 000, 1-30 (2020) Preprint 12 October 2020 Compiled using MNRAS LATEX style file v3.0. Evolution of the Earth’s Atmosphere during Late Veneer Accretion. Catriona A. Sinclair,1‹ Mark C. Wyatt,1 Alessandro Morbidelli,2 David

  10. MNRAS 000, 1–14 (2020) Preprint 8October 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/xkwy20.pdf
    8 Oct 2020: 2015).Assuming thepriors stated above,we ran LOFTI on the relative Gaia measurements until 200,000orbits were accepted, and plot the joint posterior distributions inFig. ... 160. 200. 240. []. 10 15 20. m [MJup]. m [MJup] = 1422.

  11. MNRAS 000, 1–11 (2020) Preprint 26November 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/zcac20.pdf
    26 Nov 2020: 8 A. Zurlo et al. 0 50 100 150 200 250 300Semi-major axis (au). ... Semi-major axis (au). 0. 50. 100. 150. 200. 250. Tota. l dus.

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