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11 - 20 of 24 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 24 match some words.
  1. Results that match 1 of 2 words

  2. 1906.08797

    https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf
    20 Nov 2019: temperature, and 40 K for the modified blackbody (theblackbody function is divided by 0.9 beyond 200 µm)of the disk. ... 230.02 mag 1J 1.2 5.420.03 mag 5H 1.6 5.280.04 mag 5KS 2.2 5.200.02 mag 5.
  3. MNRAS 000, 1–14 (2018) Preprint 8 January 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mybf19.pdf
    8 Jan 2019: Weoriented the disc such that the gap is narrowest towardsω 100 (PA 200). ... m. 1] NE. SW. SW-NE. 0 50 100 150 200. Deprojected distance [au].
  4. 14 Feb 2019: This uv cutoff was chosen through. 200 100 0 100 200Distance along midplane (AU). ... 006. 0.140.020.02 - -. a - 0.200.050.04 0.210.050.04 - -. β - - 0.70.20.2 - 0.40.20.2.
  5. Draft version April 2, 2019Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/dhcf19.pdf
    3 Apr 2019: 200. 300. 400 60 40 20 0 20 40 60. (b) Ring run best-fit model and residuals. ... 200. 300. 400 60 40 20 0 20 40 60. (c) ‘Skinny’ disk run best-fit model and residuals.
  6. MNRAS 000, 1–12 (2018) Preprint 4 December 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/cmfk19.pdf
    11 Apr 2019: 300 400 500 600 700 800λ (nm). 0. 100. 200. 300. ... For shock speeds of 50to 200 km/s the relative abundance of the smallest grains ismarkedly increased.
  7. MNRAS 000, 000–000 (2018) Preprint 21 February 2019 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mphp19.pdf
    21 Feb 2019: From24K and above, the average temperature of the outer discmid-plane must increase by greater than 200%.
  8. how2apply_API2018_wide copy

    https://people.ast.cam.ac.uk/~phewett/SMarkoff_2018.pdf
    15 Sep 2019: Teaching-oriented position @ university: same as above but loads can be 200 CHs!
  9. 1911.05131

    https://people.ast.cam.ac.uk/~wyatt/tw19.pdf
    20 Nov 2019: This is implemented by splitting the mass distributioninto 200 logarithmically spaced mass bins down to an arbi-trary small mass of mmin = 10. ... p. 100. 150. 200. 250. 300. 350. χ2. (a). 0.0 0.5 1.01.0.
  10. panstarrs.eps

    https://people.ast.cam.ac.uk/~wyatt/sjw19.pdf
    13 Mar 2019: 30. 0 200 400 600. Sem. imaj. or. Ax. is (. au). Time (Myrs). JupiterSaturnUranusNeptune. Figure 1. Semimajor axes (thick lines) and perihelion and aphelion.
  11. A planetesimal orbiting within the debris discaround a white ...

    https://people.ast.cam.ac.uk/~wyatt/mgeh19.pdf
    25 Apr 2019: Estimating the. constraints on the size of a planetesimal with such a periastron results in a range of 2 km < s <. 200 km with an uncertainty of 10 % in these values, ... 200 kHz. This setup provided a wavelength range of 733–1000 nm with a spectral

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