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1 - 10 of 13 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 13 match some words.

  1. Results that match 1 of 2 words

  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. vpfit10.4.dvi

    https://people.ast.cam.ac.uk/~rfc/vpfit10.4.pdf
    5 Oct 2016: VPFIT 10.4. Bob Carswell, John Webb. October 4, 2016. Contents. 1 Introduction 41.1 General terms of use. 41.2 Reference for VPFIT. 4. 2 Acknowledgements 4. 3 Obtaining the program 53.1 Download source. 53.2 Compiling and linking. 5. 4 Spectral data

  5. 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.

  6. 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.

  7. 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).

  8. 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.

  9. 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.

  10. 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.

  11. 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.

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