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1 - 10 of 15 search results for KaKaoTalk:vb20 200 |u:people.ast.cam.ac.uk where 0 match all words and 15 match some words.

  1. Results that match 1 of 2 words

  2. Astroparticle_16

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_16.pdf
    13 Mar 2012: Photon easy to detect and measure! [GeV]Tγp. 200 300 400 500 600 700. ... n=4.0 0.6 - 1.0!•MPL = 1029 200 - 100 GeV! 3/12/12 Astroparticle 23.

  3. https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120118.txt

    https://people.ast.cam.ac.uk/~wfcam/docs/minutes/minutes_120118.txt
    10 Feb 2012: He took with him an overview of what VST data for 200 band-merged ATLAS fields currently yields.

  4. Searching for Saturn's Irregular Satellite Swarm with Spitzer

    https://people.ast.cam.ac.uk/~wyatt/kwss11.pdf
    29 Jun 2012: Stansberry. OFF ON IE IW. -600 -400 -200 0 200 400 600offset (Saturn radii). ... 400. -200. 0. 200. 400. offs. et (. Sat. urn. radi.

  5. The Astrophysical Journal, 701:2019–2032, 2009 August 20…

    https://people.ast.cam.ac.uk/~wyatt/lcwm09.pdf
    1 Aug 2012: The mass of fine dust is 4 1019–2 1020 kg, equivalentto a 150–200 km radius asteroid. ... a very large particle dust population (a > 100 μm), radiatingas blackbodies at 200 K.

  6. Astroparticle_14

    https://people.ast.cam.ac.uk/~gpe/Astroparticle_14.pdf
    12 Mar 2012: GeV. ]1/. 2m. 200. 300. 400. 500. 600. (600)g. (800)g. (1000)g.

  7. 1 A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED ...

    https://people.ast.cam.ac.uk/~wyatt/jlcm12.pdf
    23 Oct 2012: 2006) and the effective. temperature of the large rubble, 200 K, they placed the dust populations at 5.8 0.6 (1) AU. ... fine dust” are much better at radiating heat and needs only to reach a color temperature of 200.

  8. mnr_20522_LR

    https://people.ast.cam.ac.uk/~wyatt/vw12.pdf
    30 Oct 2012: well. These considerations motivate us to choose f 0in increments of 30 from 0 to 330, supplemented by f 0 = [160,170, 190, 200]. ... cos 1(7/9) 160 and 360 f crit 200, which, for runaway mass loss, bound the region in which theeccentricity must

  9. ApJ409619o.dvi

    https://people.ast.cam.ac.uk/~wyatt/lwcm11.pdf
    23 Feb 2012: 2004) in amanner identical to that used for the 200 stars of the SPeX CoolStar library (Rayner et al. ... 3.2 200 0.11 350 1.62Diopside (CaMgSi2O6) 0.05 3.3 216 0.08 350 1.32.

  10. arX iv:1 201. 3622 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/ramb12.pdf
    19 Jan 2012: Each simulation was integrated for100-200 million years using the hybrid version of the Mercurycode (Chambers, 1999) with a 6 day timestep. ... 0.4. 0.8 200 Myr. Semimajor Axis (AU). Ecc. entr. icity. Log(Water Mass Fraction).

  11. arX iv:1 208. 1759 v1 [ astr o-ph .EP ...

    https://people.ast.cam.ac.uk/~wyatt/kwsp12.pdf
    9 Oct 2012: Coplanar Circumbinary Debris Disks 11. 0 50 100 150 200 250 300Semi-major axis (AU).

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