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51 - 60 of 351 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 351 match some words.

  1. Results that match 1 of 2 words

  2. Chapter 4 - Controls Reference

    https://people.ast.cam.ac.uk/~rgm/cirsi/cirsi_pixel_ir_docs_19981101/chapter4.htm
    15 Nov 1998: Base Electronics base pixel value, typically 200-1000 and is updated periodically.

  3. 1906.08797

    https://people.ast.cam.ac.uk/~wyatt/smkb19.pdf
    20 Nov 2019: temperature, and 40 K for the modified blackbody (theblackbody function is divided by 0.9 beyond 200 µm)of the disk. ... 230.02 mag 1J 1.2 5.420.03 mag 5H 1.6 5.280.04 mag 5KS 2.2 5.200.02 mag 5.

  4. DRAFT VERSION OCTOBER 25, 2022Typeset using LATEX default style ...

    https://people.ast.cam.ac.uk/~wyatt/hmsu22.pdf
    25 Oct 2022: 8. 10. 12. km/s 200 150 100 50 0 50 100 150 200Radius [au]. ... 10. 12. km/s 200 150 100 50 0 50 100 150 200Radius [au].

  5. 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.

  6. 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:.

  7. 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.

  8. 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.

  9. 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.

  10. 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

  11. 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).

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