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51 - 60 of 346 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 346 match some words.

  1. Results that match 1 of 2 words

  2. ESO Public Surveys Proposal Form Phase 1 1 Title: ...

    https://people.ast.cam.ac.uk/~rgm/vhs/v4/PS-VHS-v4p1.pdf
    5 Jun 2007: a factor of 200:1 based onthe well established space densities of the foreground L and T dwarfs. ... Observing efficiency % per tile 73.3 76.1 - - 69.9. Time for 8,200 sq deg = 5467 tiles of 1.5 sq degTotal Elapsed Hours - - 373 - 391.

  3. Microsoft PowerPoint - wyattpub

    https://people.ast.cam.ac.uk/~wyatt/wyatt_kobe06.pdf
    24 Apr 2007: Spiral structure at 200 AU implies planet at 150 AU• Same structure seen in Saturn’s rings (Charnoz et al. ... Numerical integrations of star, migrating planet, 200 planetesimalsgiving capture probabilities for 3:2 resonance:.

  4. MASS AND TEMPERATURE OF THE TWA 7 DEBRIS DISK ...

    https://people.ast.cam.ac.uk/~wyatt/mkw07.pdf
    3 Jul 2007: 2006). b >0.0096 60c Kalas et al. (2006). Eri. K2 3 730 200 40 1.5 850 0.1 85 Sheret et al. ... 2004)GJ 842.2. M0.5 20.9 200 25 4.6 850 28 5 13 Lestrade et al.

  5. Draft version March 24, 2022Typeset using LATEX twocolumn style ...

    https://people.ast.cam.ac.uk/~wyatt/hycd22.pdf
    22 Mar 2024: 6 Hull et al. 200 100 0 100 200Position along major axis (au).

  6. arX iv:1 009. 0248 v1 [ astr o-ph .SR ...

    https://people.ast.cam.ac.uk/~wyatt/sgbr10.pdf
    2 Sep 2010: 0.5. 1-50. 51-100. 101-150. 151-200. 201-250. 251-300. 301-350. 351-400. 401-450. 451-500.

  7. Submitted to ApJ 16 July 2006, Accepted 3 October ...

    https://people.ast.cam.ac.uk/~wyatt/wsgb07.pdf
    2 Nov 2006: belt width isdr = 0.5r; planetesimal strength is Q?D = 200 J kg. ... kg m3, e = 0.05, e/I = 1,Q?D = 200 J kg.

  8. ApJ accepted, 7 November 2005Preprint typeset using LATEX style ...

    https://people.ast.cam.ac.uk/~wyatt/wyat06.pdf
    19 Apr 2006: ac-count and 200 dust particles were produced with exactlythe same positions and velocities as the parent popula-tion. ... for the librationparameters to be fitted for each particle, and the meanparameters for each population of 200 dust grains to

  9. 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).

  10. Hard XMM sources

    https://people.ast.cam.ac.uk/~xmmssc/internal/xsrc_select/xsrc_hr2-err_gt0_b14.html
    28 Mar 2002: 0.901.79. A 1837. 200. 2001-02-22. Y. 2.0. -2.1. 20.6. 0. 22.4. ... 0.220.28. A 1837. 200. 2001-02-22. Y. 4.1. 0.3. 17.7. -2. 19.5.

  11. Educational and Outreach talks and activities for Carolin Crawford ...

    https://people.ast.cam.ac.uk/~csc/newcv/2011talks.html
    24 Jul 2019: Oct. 200,180. X-ray Astronomy. Talk to the National Federation of Astronomical Societies.

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