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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. 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.

  3. 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.

  4. Observing Kepler stars with WISE

    https://people.ast.cam.ac.uk/~wyatt/kw12.pdf
    7 Jul 2012: arX. iv:1. 207. 0521. v1 [. astr. o-ph. EP. ] 2. Jul 2. 012. Mon. Not. R. Astron. Soc.000, 000–000 (0000) Printed 5 July 2012 (MN LATEX style file v2.2). Confusion limited surveys: using WISE to quantify the rarit y ofwarm dust around Kepler stars.

  5. Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/jw12.pdf
    19 Jun 2012: Mon. Not. R. Astron. Soc. 000, 1–23 (2012) Printed 18 June 2012 (MN LATEX style file v2.2). Debris from terrestrial planet formation: the Moon-forming collision. Alan P. Jackson1? and Mark C. Wyatt1?1Institute of Astronomy, University of Cambridge,

  6. Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/bksm12.pdf
    5 Oct 2012: γ Tri 70 777.638.8 21.200.40 756.438.8 40 10.240.04100 718.835.5 10.290.20 708.535.5 40 11.630.04160

  7. 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

  8. midi_terr_sub3_nobold.dvi

    https://people.ast.cam.ac.uk/~wyatt/swh12.pdf
    24 Feb 2012: Mon. Not. R. Astron. Soc. 000, 1–22 (2011) Printed 24 February 2012 (MN LATEX style file v2.2). Resolving the terrestrial planet forming regions of. HD113766 and HD172555 with MIDI. R. Smith1,2, M. C. Wyatt2 and C. A. Haniff31Astrophysics Group,

  9. 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.

  10. 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.

  11. 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.

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