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1 - 10 of 14 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 14 match some words.

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  2. Draft version February 20, 2021Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/wgml21.pdf
    19 Jul 2021: 2. SpiKeS 7. ¡0:10. ¡0:05. 00:05. 0:100. 20. 40. 60. 80. ... 8 Werner et al. 2 pixel radius and a sky annulus from 12 to 20 pixels.

  3. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture10.pdf
    16 Nov 2021: 2. (T)β(10.20). We also have:. T P. ρ, T M. 2. ... 0.20 (1 0.7). M. M. ' 3.8 104 MM. (10.41). 12.

  4. Publications list for Carolin Crawford

    https://people.ast.cam.ac.uk/~csc/newcv/Full%20publications%20list%20for%20Carolin%20Crawford.pdf
    15 Feb 2021: 20. Crawford CS 1993 In Observing at a Distance eds. Emerson DT, Clowes RG,; World Scientific Publishing, p305-307 Remote observing in Edinburgh - a first-time user's view. ... 20. Fabian AC, Crawford CS, Forbes, DA, Johnstone RM 1989, Gemini, 26, 6-7

  5. MNRAS 000, 1–6 (2020) Preprint 30November 2020 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/lkmw20.pdf
    10 Feb 2021: 2 NO LUP IN CONTEXT. NO Lup (2MASS J160311.8-323920) is located in Cloud I of Lu-pus at 𝛼=16:03:11.812, 𝛿=-32:39:20.31 (J2000) ... blackbody planetesimal belt radius as 𝑅BB=3.20.3au, seeLovell et al.

  6. arX iv:2 110. 0431 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wyat21.pdf
    12 Oct 2021: However, this still means that it is onlythe brightest 20% of exozodi that have been detected, and inferences about lower dust levels have to begleaned by extrapolation. ... However, it is already clear that for 20% of stars, thelevel of dust in their

  7. Quanz_et_al_ESA_white_paper_MIR_interferometry_revised

    https://people.ast.cam.ac.uk/~wyatt/qabb21.pdf
    20 Aug 2021: Figure 1: Molecules relevant to terrestrial planet characterization between 3-20 μm (adapted from Catling et al. ... In the following we will summarize what developments from ground and space we can expect in the coming 20 years.

  8. M. Pettini: Structure and Evolution of Stars — Lecture ...

    https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture04.pdf
    7 Oct 2021: 90-120Jan 19 3754.9015 3755.2006 33 100-130Jan 20 3755.9245 3756.1993 25 90-120Jan 21 3756.9068 3757.0386 14 60-150Jan 22 3757.9004 3758.1621

  9. CO gas from the aftermath of a giant impact ...

    https://people.ast.cam.ac.uk/~wyatt/smjk21.pdf
    10 Nov 2021: This makes the presence of CO, a. highly volatile gas with sublimation temperatures as low as 20 K, extremely surprising in a. ... around a large cavity. arXiv 853, 162 (2017). 20. Morris, M.

  10. Publications of the Astronomical Society of Australia (PASA)doi:…

    https://people.ast.cam.ac.uk/~wyatt/khna21.pdf
    23 Nov 2021: Furthermore, ALMA surveys. HD (1-0) [W m-2]10 -20 10 -19 10 -18. ... The low excitationHD lines, J = 1 0, J = 2 1, are expected to havetypical widths of 5 20 km/s, dependent also on inclina-tion.

  11. MNRAS 000, 1–15 (2020) Preprint 29April 2021 Compiled…

    https://people.ast.cam.ac.uk/~wyatt/ckkm21.pdf
    29 Apr 2021: 2013); itwas not spatially resolvedbut a temperature of 24K and radius of 20-40 auwere estimated. ... Δ𝜒2 0 2 20. ΔBIC 0 42 40. 6” 4” 2” 0” -2” -4” -6”RA Offset.

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