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1 - 10 of 42 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 42 match some words.

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  2. Draft version January 1, 2018Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mwoa18.pdf
    2 Jan 2018: 2). 6 Matrà et al. 20 10 0 10 20v-v (km/s). ... 20 10 0 10 20v-v (km/s). 8. 6. 4. 2. 0.

  3. arX iv:1 801. 0542 9v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kmmp18.pdf
    18 Jan 2018: n 20. 18Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 18 January 2018 (MN LATEX style file v2.2). ... Acke et al. 2012; MacGregor et al. 2017). For β Pic and HR 4796A, these observations are made atthe 10 to 20 million-year age that places

  4. MNRAS 000, 1–16 (2017) Preprint January 22, 2018 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rwmk18.pdf
    22 Jan 2018: P] 1. 9 Ja. n 20. 18. 2 M. J. Read et al.

  5. The picture shows the evolution of a thin representative ...

    https://people.ast.cam.ac.uk/~haehnelt/rtnigmwebbackup/reion/figcaption1.html
    24 Jan 2018: The picture shows the evolution of a thin representative slice of the universe (4 Mpc/h x 4 Mpc/h comoving) as a function of time (represented as a scale factor a). The evolution starts at z20 (a0.05) and stops at z=4 (a=0.2). The respective panels

  6. Detection of HeII reionization, due to its effect on ...

    https://people.ast.cam.ac.uk/~haehnelt/rtnigmwebbackup/reion/figcaption5.html
    24 Jan 2018: The hashed region for the simulation delineates the 20 and 80 per centile of bootstrap re-sampled mock samples.

  7. Analysis of the Herschel DEBRIS Sun-like star sample

    https://people.ast.cam.ac.uk/~wyatt/skwl18.pdf
    19 Feb 2018: 3040. N. 0 10 20 30 40N. F spectral typeG spectral typeK spectral typeDUNES target. ... 20. 30. 40. 50. 60. 70. Num. ber. F spectral typeG spectral typeK spectral type.

  8. arX iv:1 803. 0283 2v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/kbae18.pdf
    9 Mar 2018: 160µm. 20 10 0 -10 -20α cos δ offset ("). GJ 3634, nearby sources. ... 100µm -0.20. -0.12. -0.03. 0.05. 0.13. 0.22. 0.30. mJy. arc. sec-.

  9. Gaia DFS PLS prop

    https://people.ast.cam.ac.uk/~gil/Gaia-RAeS-Leslie-Bedford-April2017.pdf
    29 Mar 2018: NEO/Atira Earth-crossing? 20. The Sun and stars distort space-time and the path of light. ... Slide Number 20. Slide Number 21. Slide Number 22. Tracking stardust: origins of the chemical elements.

  10. arX iv:1 803. 1126 5v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/edhm18.pdf
    2 Apr 2018: 88230 GJ 380 -0.111 0.059 -0.077 0.056 20 -0.189 0.087 13 pix 2.59104 -299 217 -1.4.

  11. Draft version April 5, 2018Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/mmkw18.pdf
    5 Apr 2018: are derived assuming stars have reached themain-sequence, using tabulated values from Pecaut & Mamajek (2013), for all stars older than 20 Myr except low-mass AUMic, which is still pre-main ... 2015). For stars younger. than 20 Myr, we use values from

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