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1 - 12 of 12 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 12 match some words.

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  2. Astronomy & Astrophysics manuscript no. letter_HD206893 c©ESO…

    https://people.ast.cam.ac.uk/~wyatt/mhcc16.pdf
    2 Dec 2016: Zuckerman & Song(2004) estimated an age of 200 Myr based on X ray, radial ve-locity and proper motion measurements. ... Us-ing an age of 200 Myr (respectively 800 Myr, 2 Gyr) and theAMES-Cond models (Baraffe et al.

  3. MNRAS 000, 1–6 (2016) Preprint 13 July 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/agwk16.pdf
    13 Jul 2016: 0 100 200 300 400 500. UV Distance [kλ]. 100. 0. ... 100. 200. 300. Re(v. ) [m. Jy]. 0 100 200 300 400.

  4. Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf
    21 Jul 2016: A 200 km/svelocity range is shown around the stellar velocity in the heliocen-tric frame of 23.0 0.3 km/s (Torres et al. ... The wide-fit baseline yields a 10.5 sigma detection of 200.0 19.1 mK km/s.

  5. Draft version December 23, 2016Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/cmws17.pdf
    23 Dec 2016: 100. 0. 100. 200. 300. 2.''. 118.AU. N. E. NICMOS, F110WALICE program. ... 2. 4. 1.10-6. 0.00001. 5.10-6. 200 100 0 100 200. 15.

  6. MNRAS 000, 1–21 (2016) Preprint 23 September 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mdwk16.pdf
    23 Sep 2016: 4 L. Matrà et al. -200 -100 0 100 200. -60-40-20. ... 1. CO J=2-1N. E. -200 -100 0 100 200Stellocentric distance (AU).

  7. MNRAS 000, 1–12 (2015) Preprint 12 May 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mmsw16.pdf
    17 May 2016: The presented im-ages are the median of 200 iterations. We observe a noise level of. ... Moreover, the value of Ṁ ishighly dependant on Q?D which could vary between 200 and 10.

  8. arX iv:1 604. 0828 6v1 [ast ro-p h.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/mcbe16.pdf
    29 Apr 2016: 2011). This deficit was interpreted asbeing the result of emission originating within the field ofview ( 200 mas), but at spatial scales of several stellarradii, i.e.

  9. MNRAS 000, 1–22 (2016) Preprint 7 November 2016 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/mwpm16.pdf
    7 Nov 2016: off. set [. arcs. ec]. -100 -50 0 50 100 150 200 250Intensity [µJy beam1]. ... 0. 100. 200. Inte. nsity. [µJy. bea. m. 1]. i). -4.

  10. arX iv:1 601. 0686 6v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/dhmh16.pdf
    27 Jan 2016: 600. -400. -200. 0. 200. 400. 600. Flux. [A. DU. ]. 0 20 40 60 80 100 120Number of occurence. AVG: 0.4RMS: 155.6.

  11. Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kwcp16.pdf
    7 Jun 2016: Mon. Not. R. Astron. Soc. 000, 1–16 (2002) Printed 7 June 2016 (MN LATEX style file v2.2). A self-consistent model for the evolution of the gasproduced in the debris disc of β Pictoris. Q. Kral?, M. Wyatt, R. F. Carswell, J. E. Pringle, L. Matrà

  12. Space Science Reviews manuscript No.(will be inserted by the ...

    https://people.ast.cam.ac.uk/~wyatt/wj16.pdf
    15 Mar 2016: Space Science Reviews manuscript No.(will be inserted by the editor). Insights into planet formation from debris disks. II. Giant impacts in extrasolar planetary systems. Mark C. Wyatt Alan P. Jackson. Received: date / Accepted: date. Abstract Giant

  13. arX iv:1 610. 0071 4v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/wbjm16.pdf
    7 Oct 2016: arX. iv:1. 610. 0071. 4v1. [as. tro-. ph.E. P] 3. Oct. 201. 6. MNRAS 000, 1–25 (2016) Preprint 5 October 2016 Compiled using MNRAS LATEX style file v3.0. How to design a planetary system for different scattering. outcomes: giant impact sweet spot,

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