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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. 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

  3. 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.

  4. 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).

  5. 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

  6. 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.

  7. 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.

  8. 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.

  9. 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,

  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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